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Sample search results for: ab doradus moving

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1 The Astrophysical Journal, 731:91 (15pp), 2011 April 20 doi:10.1088/0004-637X/731/2/91 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
 

Summary:  OF GIANT H ii REGIONS?: A STUDY OF STELLAR FEEDBACK IN 30 DORADUS Laura A. Lopez1 , Mark R. Krumholz1... region 30 Doradus in the Large Magellanic Cloud. We exploit high-resolution, multi-wavelength images... the implications of a dominant radiation pressure on the early dynamics of 30 Doradus. Key words: galaxies: star

  

Source: Berkeley Illinois Maryland Association (BIMA)

 

Collection: Physics

 
2 D. Montes1, J. Lpez-Santiago1,2, I. Crespo-Chacn1, R.M. Martnez-Arniz1, J. Maldonado1,3
 

Summary:  possible members of the nearby young moving group AB Doradus. We have used high resolution echelle... ). Taking this into account, they propose an age range of 75­150 Myr for all the MG. AB Doradus Moving Group... Fig. 5: High resolution spectra of possible members ...

  

Source: Gutiérrez, David Montes - Facultad de Ciencias Físicas, Universidad Complutense de Madrid

 

Collection: Physics

 
3 ULTRAVIOLET OBSERVATIONS OF STARS IN THE MAGELLANIC CLOUDS: A HISTORICAL BRIDGE FROM THE SUN TO R 136 AND BEYOND
 

Summary:  named Henry, who pushed the short wavelength limit of the solar spectrum to 3047 š A (Draper 1873a,b... , Cornu moved down another hundred angstroms by measuring the solar spectrum to 2947 š A near sea level... 1940 N 51 NGC 2014 NGC 2032 SN 1987A N 49 N 70 30 Doradus N 4 N 79 N 11 N 113 N 119 N 132 Sk ­67 78 NGC

  

Source: Parker, Joel Wm. - Department of Space Studies, Southwest Research Institute

 

Collection: Physics

 
4 High resolution spectroscopic analysis of cool stars possible members of the AB Doradus
 

Summary:  High resolution spectroscopic analysis of cool stars possible members of the AB Doradus moving... B4) 2 AB Doradus Moving Group In recent years, a series of young stellar kinematic groups of late... resolution spectra of possible members of the AB ...

  

Source: Gutiérrez, David Montes - Facultad de Ciencias Físicas, Universidad Complutense de Madrid

 

Collection: Physics

 
5 Spectroscopic EUVE Observations of the Active Star AB Doradus
 

Summary:  Spectroscopic EUVE Observations of the Active Star AB Doradus By SLAVEK M. RUC I NSK I 1 , ROLF... ­rotating (0.515 day) late­type star, AB Doradus (HD 36705), made by the Extreme Ultraviolet Explorer (EUVE... ­Main Sequence objects in the solar neighborhood, with an inferred age of 10 6\Gamma7 years. ...

  

Source: White, Stephen - Department of Astronomy, University of Maryland at College Park

 

Collection: Physics

 
6 L-band (3.5 m) IR-excess as an Indicator of Circumstellar Disks
 

Summary:  Doradus 12 6.2. RCW 57 13 6.3. Galactic Centre 15 6.4. RCW 38 16 PART 2: THE DATA 17 7. Observations 17 7... . Analysis of results 38 9.1. Colour-colour diagrams 38 9.2. Interstellar reddening 38 9.3. 30 Doradus... and RCW 57 ­ Infrared excess 39 9.4. 30 Doradus and RCW 57 ­ spatial distribution 44 9.5. Contamination

  

Source: Stockholm Observatory

 

Collection: Physics

 
7 D. Montes1, J. Lpez-Santiago1,2, I. Crespo-Chacn1, R.M. Martnez-Arniz1, J. Maldonado1,3
 

Summary:  spectra of possible members of the AB Doradus moving group in the H and LiI 6708 Å line region. Note... . AB Doradus and B4 Moving Group Pic Moving Group Tuc-Hor Moving Group Acknowledgments This work... possible members of ...

  

Source: Gutiérrez, David Montes - Facultad de Ciencias Físicas, Universidad Complutense de Madrid

 

Collection: Physics

 
8 8th Cool Stars, Stellar Systems and the Sun 1 A SEARCH FOR RADIO EMISSION IN THE ff PERSEI CLUSTER
 

Summary:  activity might be expected in these stars by analogy with the similar star AB Doradus. THE OPEN CLUSTER ff... The example of the active southern star AB Doradus makes us somewhat sur­ prised not to have detected any... Dor, are less active as radio emitters than AB Dor. If ...

  

Source: White, Stephen - Department of Astronomy, University of Maryland at College Park

 

Collection: Physics

 
9 A dynamical calibration of the mass luminosity relation at very low stellar
 

Summary:  AB Doradus A. Here we report a dynamical determination of the mass of the newly resolved low... for planetary mass companions. The K1 star AB Doradus A has long been of great interest owing to its proximity... Dor moving group', which has an age of 50 Myr (refs 8, 13). ...

  

Source: Steward Observatory, Center for Astronomical Adaptive Optics

 

Collection: Physics

 
10 A&A 462, 615620 (2007) DOI: 10.1051/0004-6361:20066208
 

Summary:  , and conclude that the AB Dor moving group #12;618 M. Janson et al.: Improved age constraints for the AB Doradus... Improved age constraints for the AB Doradus quadruple system (Research Note) The binary nature of AB... : fundamental parameters ­ ...

  

Source: Steward Observatory, Center for Astronomical Adaptive Optics

 

Collection: Physics

 
11 The X--ray Spectra of Flares from AB Doradus Stephen M. White
 

Summary:  The X--ray Spectra of Flares from AB Doradus Stephen M. White Dept. of Astronomy, University... Institute of Astronomy and Astrophysics, Academica Sinica, Taipei AB Doradus is a rapidly--rotating K0 dwarf... a 40 ksec pointing on AB Dor in 1993 November during which it initially showed a ...

  

Source: White, Stephen - Department of Astronomy, University of Maryland at College Park

 

Collection: Physics

 
12 A&A 446, 733738 (2006) DOI: 10.1051/0004-6361:20053757
 

Summary:  On the dynamics of the AB Doradus system J. C. Guirado1, I. Martí-Vidal1, J. M. Marcaide1, L. M. Close2, J. C... and they constitute the quadruple AB Doradus system. From the astrometric data available at different wavelengths, we... .1051/0004-6361:20053757 #12;734 J. C. Guirado et al.: On the dynamics of ...

  

Source: Steward Observatory, Center for Astronomical Adaptive Optics

 

Collection: Physics

 
13 ABUNDANCES AND FLARES IN THE ASCA OBSERVATION OF THE YOUNG K0 STAR AB DORADUS
 

Summary:  ABUNDANCES AND FLARES IN THE ASCA OBSERVATION OF THE YOUNG K0 STAR AB DORADUS Stephen M. WHITE Dept... Abstract The ASCA observation of the young, rapidly--rotating active K0 dwarf AB Doradus showed very steady... . Introduction AB Doradus is a very active nearby ...

  

Source: White, Stephen - Department of Astronomy, University of Maryland at College Park

 

Collection: Physics

 
14 A&A manuscript no. (will be inserted by hand later)
 

Summary:  offprint requests to: R. Mewe 1. Introduction AB Doradus (HD 36705, spectral type K0­2 IV­V) is one... is present, this #12; 2 R. Mewe et al.: EUVE & ASCA observations of AB Doradus means that active regions... --known #12; R. Mewe et al.: EUVE & ASCA observations of AB ...

  

Source: White, Stephen - Department of Astronomy, University of Maryland at College Park

 

Collection: Physics

 
15 Astron. Nachr. / AN 326, No. 10, 10331039 (2005) / DOI 10.1002/asna.200510442 AB Doradus C: age, spectral type, orbit, and comparison to
 

Summary:  Astron. Nachr. / AN 326, No. 10, 1033­1039 (2005) / DOI 10.1002/asna.200510442 AB Doradus C: age... A, Weinheim #12;E.L. Nielsen et al.: AB Doradus C: age, spectral type, orbit, and comparison to evolutionary... -VCH Verlag GmbH & Co. KGaA, Weinheim #12;E.L. Nielsen et al.: AB ...

  

Source: Steward Observatory, Center for Astronomical Adaptive Optics

 

Collection: Physics

 
16 NEW PHOTOMETRY AND SPECTRA OF AB DORADUS C: AN ACCURATE MASS DETERMINATION OF A YOUNG LOW-MASS OBJECT WITH THEORETICAL EVOLUTIONARY TRACKS1
 

Summary:  MASS FOR AB DORADUS C 739 #12;fitted the ``continuum'' with a polynomial and attempted to re- move... NEW PHOTOMETRY AND SPECTRA OF AB DORADUS C: AN ACCURATE MASS DETERMINATION OF A YOUNG LOW... -- stars: individual (AB Doradus C) -- stars: ...

  

Source: Steward Observatory, Center for Astronomical Adaptive Optics

 

Collection: Physics

 
17 New Astronomy 7 (2002) 3543 www.elsevier.com/locate/newast
 

Summary:  ; Stars: individual: AB Doradus; Stars: individual: AU Microscopii; Radio continuum: stars; Techniques... V824 Arae, HR 1099, AB Doradus tions (cf. Lestrade et al., 1986; Mutel et al., 1986; and AU... ­50 38­48 3569 0.72 15612 24/8/94 454 34.92 47­53 37­42 88628 0.74 6265 (e) AB ...

  

Source: White, Stephen - Department of Astronomy, University of Maryland at College Park

 

Collection: Physics

 
18 THE SPECTRUM OF INTEGRATED MILLIMETER FLUX OF THE MAGELLANIC CLOUDS AND 30 DORADUS FROM TOPHAT AND DIRBE DATA
 

Summary:  THE SPECTRUM OF INTEGRATED MILLIMETER FLUX OF THE MAGELLANIC CLOUDS AND 30 DORADUS FROM TOPHAT... Doradus (the Tarantula Nebula) in the LMC in four frequency bands centered at 245, 400, 460, and 630 GHz... and SMC. We report separate results for the LMC with the active star-forming region 30 Doradus (the

  

Source: Aguirre, James E. - Department of Physics and Astronomy, University of Pennsylvania; Timbie, Peter - Department of Physics, University of Wisconsin at Madison

 

Collection: Physics

 
19 ASCA X--ray Spectra of Quiescent and Flaring Emission from AB Doradus
 

Summary:  ASCA X--ray Spectra of Quiescent and Flaring Emission from AB Doradus S. M. White 1 , R... --rotating K dwarf AB Doradus with ASCA in November 1993. The star's X--ray flux was essentially steady... \Theta 10 30 ergs s \Gamma1 (0.5--10 keV). At the flare peaks, LX (? 0.5 keV)/L bol = .002. ...

  

Source: White, Stephen - Department of Astronomy, University of Maryland at College Park

 

Collection: Physics

 
20 ASP Conference Series, Vol. **VOLUME**, **PUBLICATION YEAR** **EDITORS**
 

Summary:  Doradus The nearby K0 V star AB Doradus is a kinematic member of the Pleiades moving group (Innis et al... of Three Very Active Stars: AB Dor, 44i Boo, and #27; 2 CrB Je#11;rey L. Linsky and Steve Skinner JILA... (44i Boo), and a Pleiades-age K0 dwarf (AB Dor). The ...

  

Source: Linsky, Jeffrey L. - JILA & Center for Astrophysics and Space Astronomy, University of Colorado at Boulder

 

Collection: Physics


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21 Astronomy & Astrophysics manuscript no. 272230do April 28, 2005 (DOI: will be inserted by hand later)
 

Summary:  later) L-band (3.5 µm) IR-excess in massive star formation I. 30 Doradus M. Maercker1,2 and M. G. Burton... @phys.unsw.edu.au Received January 18, 2005; accepted April 18, 2005 Abstract. L-band data of 30 Doradus at 3.5 µm taken... detected at L-band in 30 Doradus have an IR-excess. Key words. Stars: circumstellar matter, ...

  

Source: Burton, Michael - School of Physics, University of New South Wales

 

Collection: Physics

 
22 Mon. Not. R. Astron. Soc. 000, 000{000 (0000) Printed 18 January 2002 (MN L A T E X style le v2.2) The global magnetic topology of AB Doradus
 

Summary:  .2) The global magnetic topology of AB Doradus M. Jardine 1 , ? A. Collier Cameron 1 & J.-F. Donati 2 1 School... 0000 RAS, MNRAS 000, 000{000 #12; Magnetic topology of AB Doradus 3 Figure 3. Images of the combined... RAS, MNRAS 000, 000{000 #12; Magnetic topology of AB ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
23 Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 29 October 2001 (MN LATEX style file v1.4) Modelling surface magnetic field evolution on AB Dorad^us
 

Summary:  .4) Modelling surface magnetic field evolution on AB Dorad^us due to diffusion and surface differential rotation... -rotating K0 dwarf AB Dorad^us, we have created a potential approximation to the observed radial magnetic... INTRODUCTION AB Dorad^us is a K0 dwarf, ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
24 **Volume Title** ASP Conference Series, Vol. **Volume Number**
 

Summary:  ­52 381 B (aka GSC 08047­00232), 2MASS J01415823­4633574. · AB Doradus: HD 89744 B. Our sample also... , Tucana-Horologium and AB Doradus. Taking into account our previous results of contamination by old field... ** Astronomical Society of the Pacific Kinematics of ultracool dwarfs: Membership in ...

  

Source: Gutiérrez, David Montes - Facultad de Ciencias Físicas, Universidad Complutense de Madrid

 

Collection: Physics

 
25 A CORONAGRAPHIC IMAGING SEARCH FOR PLANETARY MASS COMPANIONS TO NEARBY YOUNG STARS USING THE NEAR INFRARED CAMERA ON THE HUBBLE SPACE TELESCOPE. J. Farihi1
 

Summary:  ), the Tucana/HorA group (d 45 pc, 30 Myr), and the AB Doradus group (d 20 pc, 50 Myr). The ages... groups; the TW Hydrae Association (d 60 pc, 8 Myr), the Pictoris moving group (d 35 pc, 12 Myr

  

Source: Schneider, Glenn - Department of Astronomy, University of Arizona

 

Collection: Physics

 
26 TimeVariable Photo-Evaporation of
 

Summary:  for disks formed at the same time in the same cluster. #12;30 Doradus: 100+ O/B stars Photo... . But we know that stars move quickly, with many cluster crossings in first several Myr. #12;We performed N

  

Source: Throop, Henry - Department of Space Studies, Southwest Research Institute

 

Collection: Physics

 
27 Ultraviolet Imaging Telescope Observations of the Magellanic Clouds Joel Wm. Parker, 1 Jesse K. Hill, 2 Robert Cornett, 2 Joan Hollis, 2 Emily Zamkoff, 2 Ralph C. Bohlin, 3
 

Summary:  in the SMC were obtained. Populous regions (e.g., 30 Doradus, NGC 330, NGC 346, N 11, and N 51), as well... obtained ex­ posure times in the Clouds up to three times longer. Some fields such as the 30 Doradus and SN... ?,84,85,86?,90,98­103,104?, 39,43­45,47,49?,53? ``Field 4'' 106,111,114?,119,120,124? LMC --- 30 Doradus East ...

  

Source: Parker, Joel Wm. - Department of Space Studies, Southwest Research Institute

 

Collection: Physics

 
28 Mon. Not. R. Astron. Soc. 338, 687710 (2003) Heavy elements in Galactic and Magellanic Cloud H II regions
 

Summary:  3576 and of the Magellanic Cloud H II regions 30 Doradus, LMC N11B and SMC N66, recording the optical... recombination lines (ORLs) of C II, N II and O II. A spatial analysis of 30 Doradus is performed, revealing... al. 2000; Liu 2002a,b; P´equignot et al. 2002a,b). The exact nature and origin of the ...

  

Source: Liu, Xiaowei - Kavli Institute for Astronomy and Astrophysics, Peking University

 

Collection: Physics

 
29 Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 7 May 1998 (MN L a T E X style file v1.4) Latitude distributions and lifetimes of starspots on G
 

Summary:  in the Hff profile attributable to prominence features, similar to those seen on AB Doradus (Collier Cameron... echelle spectra to produce magnetic and surface brightness reconstructions of the K0 dwarf AB Doradus... & Collier Cameron (1997) have measured the differ­ ential rotation rate of the K0 dwarf ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
30 MAD Science Demonstration Proposal R136: The young massive star cluster at the core of 30 Doradus
 

Summary:  MAD Science Demonstration Proposal R136: The young massive star cluster at the core of 30 Doradus... imaging of R136, the dense star cluster at the centre of the 30 Doradus starburst region. The exquisite... Case: 30 Doradus is one of the largest star-forming regions in the Local Group. At its core

  

Source: Liske, Jochen - European Southern Observatory

 

Collection: Physics

 
31 Beauty and Astrophysics Michael S. Bessell
 

Summary:  from external galaxies to our galaxy, the Milky Way, then move along the galact* *ic plane from... * *tion in the bar 4c LMC zoom BO3Hff Nikon msb 30 Doradus and shells of HII regions d... * *ominate this image. 5a 30 Doradus BVR 40 inch sung Three beautiful views of 30 Doradus. S

  

Source: Bessell, Mike - Mt. Stromlo Observatory & Research School of Astronomy and Astrophysics, Australian National University

 

Collection: Physics

 
32 Beauty and Astrophysics Michael S. Bessell
 

Summary:  are presented in a somewhat arbitrary progression from external galaxies to our galaxy, the Milky Way, then move... msb HII regions and the old stellar population in the bar 4c LMC zoom BO3Hff Nikon msb 30 Doradus... and shells of HII regions dominate this image. 5a 30 Doradus BVR 40 inch sung Three beautiful views of 30

  

Source: Bessell, Mike - Mt. Stromlo Observatory & Research School of Astronomy and Astrophysics, Australian National University

 

Collection: Physics

 
33 arXiv:astroph/0111235 Mon. Not. R. Astron. Soc. 000, 000{000 (0000) Printed 14 November 2001 (MN L A T E X style le v2.2)
 

Summary:  ;erential rotation on AB Doradus A. Collier Cameron 1 ? , J.-F. Donati 2 1 School of Physics and Astronomy... of individual starspots on the rapidly rotating young K0 dwarf AB Doradus, at six epochs between 1988 December... .cameron@st-and.ac.uk rotating K0 dwarf AB ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
34 Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 13 November 2001 (MN LATEX style file v2.2) Doin' the twist: Secular changes in the surface differential
 

Summary:  .2) Doin' the twist: Secular changes in the surface differential rotation on AB Doradus A. Collier Cameron1... rotating young K0 dwarf AB Doradus, at six epochs between 1988 December and 1996 December. The equatorial... .cameron@st-and.ac.uk rotating K0 dwarf AB ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
35 Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 8 March 1999 (MN L A T E X style file v1.4) The potential magnetic field of AB Doradus: comparison
 

Summary:  .4) The potential magnetic field of AB Doradus: comparison with Zeeman­Doppler images. Moira Jardine 1 ,John R... , MNRAS 000, 000--000 #12; Magnetic field of AB Doradus 5 Figure 3. Peak values of the cross... topology of the young, rapidly­rotating K0 dwarf AB Dor by assuming that the ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
36 Mon. Not. R. Astron. Soc. 000, 120 (2010) Printed 8 July 2010 (MN LATEX style file v2.2) The R136 star cluster hosts several stars whose individual masses
 

Summary:  % of the ionizing flux of the entire 30 Doradus region. Comparisons with stellar models calculated for the main... cluster of the Tarantula nebula (30 Doradus) within the Large Magellanic Cloud (LMC). R136 is sufficiently... and 30 Doradus. Finally, Table 1. Log of spectroscopic observations of R136 and NGC 3603 stars used

  

Source: Dworetsky, Mike - University of London Observatory & Department of Physics and Astronomy, University College London

 

Collection: Physics

 
37 Physics and Astronomy Michigan State University Fall 2006
 

Summary:  and is expected to play a major leadership role as we slowly move our main research emphasis in experimental... -time leader of our CTEQ effort, has moved to Seattle to spend more time with his grandchildren. Harry Weerts... is available at xxx.lanl.gov/abs/astro-ph/0611827. The Link between Quasars and the Evolution of Galaxy

  

Source: Michigan State University, Center for Beam Theory and Dynamical Systems

 

Collection: Physics

 
38 Radio Emission from Cool Stars Stephen M. White
 

Summary:  . A notable example is the K0 star AB Doradus. Lim et al. (1992,1994) find that it shows clear rotational... --hemisphere stars AB Doradus and HD 32918. AB Dor (K0) and its common--proper--motion M dwarf companion Rst 137B... binaries; fl, RS CVn binaries; ffi, RS CVn binaries containing ...

  

Source: White, Stephen - Department of Astronomy, University of Maryland at College Park

 

Collection: Physics

 
39 Formation of the Galactic Halo .... Inside and Out ASP Conference Series, Vol. 92, 1996
 

Summary:  cluster formation in the halo was completed (Larson 1990a,b, 1992b). Although our Galaxy has evidently... in the entire Local Group, NGC 2070 at the center of the giant 30 Doradus H II region. It has recently become... globular cluster. It is noteworthy also that the 30 Doradus star-forming complex is itself unique in being

  

Source: Larson, Richard B. - Department of Astronomy, Yale University

 

Collection: Physics

 
40 TRANSIT SURVEY OF THE OPEN CLUSTER M37. II. VARIABLE STARS J. D. Hartman,2
 

Summary:  , including a previously identified variable that we suggest is probably a hybrid Doradus/ Scuti pulsator... Doradus pulsating component (only the second such variable found in an eclipsing binary), and a low... parameters for the DEB+ Doradus system yields MP ¼ 1:58 Æ 0:04 M, MS ¼ 1:58 Æ 0:04 M, RP ¼ 1:39 Æ 0:07 R

  

Source: Gaudi, B. Scott - Department of Astronomy, Ohio State University

 

Collection: Physics


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41 From Cosmic Dawn to Our Solar System: A Next-Generation UVOptical Space Facility for the Study of Star Formation
 

Summary:  ­ Image of the 30 Doradus complex within the LMC. Overlayed are the field of view of the wide... ) varies with the mode of star formation and metallicity. Tier 2 Moving outward, we will conduct a complete... -regions like 30 Doradus differ from more modest H II-regions within the Milky Way, and (5) determine the impact

  

Source: Jansen, Rolf Arthur - Department of Physics and Astronomy, Arizona State University

 

Collection: Physics

 
42 THE MESSENGER No. 12-March 1978
 

Summary:  telescope in a blink microscope, he noticed a small trail of a moving 18th-magnitude object. From... the orbit, and it is now known that 1977 UB is a unique object in the solar system. It moves in a rather... occasions and the images are therefore somewhat fuzzy, in particular on the 10th. But it does not move

  

Source: Liske, Jochen - European Southern Observatory

 

Collection: Physics

 
43 The nearest young moving groups J. Lopez-Santiago1,2
 

Summary:  .84 6 207129a 21 48 15.75 -47 18 13.01 G0 V 15.6 -6.5 1.3 -13.3 -22.2 0.3 0.60 0.66 - AB Doradus Moving... ) or the recently discovered AB Doradus MG (Zuckerman et al. 2004). The location of these young MGs inside the Local... . (2004) have identified a new group of stars ...

  

Source: Gutiérrez, David Montes - Facultad de Ciencias Físicas, Universidad Complutense de Madrid

 

Collection: Physics

 
44 Starburst Galaxies Observed With the Hubble Space Telescope
 

Summary:  region of 30 Doradus in the Large Magellanic Cloud (see p. xi of Leitherer et al. 1991) --- a star... 100 times as luminous as the 30 Doradus region and has an age of 4 -- 5 Myr. Massive­star formation... , indirect techniques, rather than on a stellar census. The central region of 30 Doradus is one of the few

  

Source: Space Telescope Science Institute, Starburst and Galaxy Evolution Group

 

Collection: Physics

 
45 The nearest young moving groups J. LopezSantiago 1,2 , D. Montes 2 , I. CrespoChacon 2 and M.J. FernandezFigueroa 2
 

Summary:  .3 ­13.3 ­22.2 0.3 0.60 0.66 ­ AB Doradus Moving Group 1405 00 18 20.90 30 57 22.03 K2 V 30.6 ­11.2 0... ) or the recently discovered AB Doradus MG (Zuckerman et al. 2004). The location of these young MGs inside the Local... In Table 1 we list the stars belonging to the nearest ...

  

Source: Osservatorio Astronomico Di Palermo, Giuseppe S. Vaiana

 

Collection: Physics

 
46 tel-00152441,version1-6Jun2007 tel-00152441,version1-6Jun2007
 

Summary:  .3 ­13.3 ­22.2 0.3 0.60 0.66 ­ AB Doradus Moving Group 1405 00 18 20.90 30 57 22.03 K2 V 30.6 ­11.2 0... ) or the recently discovered AB Doradus MG (Zuckerman et al. 2004). The location of these young MGs inside the Local... In Table 1 we list the stars belonging to the nearest ...

  

Source: Ecole Polytechnique, Centre de mathématiques

 

Collection: Mathematics

 
47 THE ASTROPHYSICAL JOURNAL, 498:735756, 1998 May 10 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
 

Summary:  ), (2, 1) S(1), andH 2 H 2 (5, 3) O(3) lines and the 12CO J \ 1 ] 0 line from 30 Doradus and N159/N160... Doradus (0, 0) position (see the object list in andTable 3), telluric OH lines. The OH (9, 7) (j \ 2... ) position of 30 Doradus in units of 10~8 ergs s~1 cm~2 sr~1 (kmH 2s~1)~1. The smooth curve shows a Ðt

  

Source: Pak, Soojong - Department of Astronomy and Space Science, Kyung Hee University

 

Collection: Physics

 
48 The AGN dance: astrometric variability as the result of supernova explosions in nuclear
 

Summary:  remnant. Thus, a strong prediction of the model is that the BLR of low luminosity AGN should move... be observed to move around the center of the cluster. We will refer to this predicted astrometric variability... of 30 Doradus (Malamuth and Heap 1994) indicate that the IMF in the core of the prototype starburst 30

  

Source: Aretxaga, Itziar - Instituto Nacional de Astrofísica Óptica y Electrónica

 

Collection: Physics

 
49 The Astronomical Journal, 142:155 (13pp), 2011 November doi:10.1088/0004-6256/142/5/155 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
 

Summary:  % were likely pulsating stars. The latter category includes Scuti, Doradus, and RR Lyrae variables. One... the telescopes are fixed, stars move in circles about the center of the CCD but only traverse a tiny fraction... , Scuti variable; EC, contact binary; ESD, semi-detached binary; ED, detached binary; GDOR, Doradus

  

Source: Ashley, Michael C. B. - School of Physics, University of New South Wales

 

Collection: Physics

 
50 Imaging the magnetic topologies of cool active JeanFrancois Donati
 

Summary:  lines with Least­Squares Deconvolution) for the rapidly rotating young K0 dwarf AB Doradus (Donati et al... of the ultra fast rotator AB Doradus (see Fig. 14, Donati et al. 1999a). We speculate that the toroidal... fast rotator AB Doradus, derived from the Stokes V ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
51 A&A 365, L336--L343 (2001) DOI: 10.1051/00046361:20000220
 

Summary:  The XMM­Newton view of stellar coronae: X­ray spectroscopy of the corona of AB Doradus # M. G˜udel 1 , M... November 2000 Abstract. We report results of deep X­ray observations of AB Doradus obtained with the XMM... : coronae -- stars: flare -- stars: individual: AB ...

  

Source: University College London - Mullard Space Science Laboratory

 

Collection: Physics

 
52 A&A 365, L336L343 (2001) DOI: 10.1051/0004-6361:20000220
 

Summary:  The XMM-Newton view of stellar coronae: X-ray spectroscopy of the corona of AB Doradus M. G¨udel1, M... report results of deep X-ray observations of AB Doradus obtained with the XMM-Newton obser- vatory during... : individual: AB Doradus ­ X-rays: stars 1. ...

  

Source: Audard, Marc - INTEGRAL Science Data Centre & Observatory of Geneva, Université de Genève

 

Collection: Physics

 
53 F090Mmag = +22.3 0.35 F110Mmag = +20.61 0.15 F160Wmag = 18.24 0.02 F090M = +7.14 0.35 110M = +7.02 0.15 F160W = + 4.98 0.11
 

Summary:  , age ~ 30 Myrs) D) AB Doradus group (d ~ 20 pc, age ~ 50 Myrs) Ages of these young nearby stellar... , age ~ 8 Myrs) B) Pictoris moving group (d ~ 35 pc, age ~ 12 Myrs) C) Tucana/HorA group (d ~ 45 pc

  

Source: Schneider, Glenn - Department of Astronomy, University of Arizona

 

Collection: Physics

 
54 Astronomy & Astrophysics manuscript no. (will be inserted by hand later)
 

Summary:  of stellar coronae: X-ray spectroscopy of the corona of AB Doradus ? M. Gudel 1 , M. Audard 1 , K. Briggs 2... report results of deep X-ray observations of AB Doradus obtained with the XMM-Newton obser- vatory during... { stars: are { stars: individual: AB Doradus ...

  

Source: Guedel, Manuel - Institut für Astronomie, Universität Wien

 

Collection: Physics

 
55 Astron. Nachr. / AN 331, No. 9/10, 989 992 (2010) / DOI 10.1002/asna.201011443 Kepler observations: Light shed on the hybrid Doradus Scuti
 

Summary:  observations: Light shed on the hybrid Doradus ­ Scuti pulsation phenomenon A. Grigahc`ene1, , K... Scuti stars ­ gamma Doradus stars Through the observational study of stellar pulsations, the internal... structure of stars can be probed and theoretical models can be tested. The main sequence Doradus (Dor

  

Source: Monteiro, Mário João - Centre for Astrophysics, University of Porto

 

Collection: Physics

 
56 Mon. Not. R. Astron. Soc. 000, 000--000 (0000) Printed 25 January 2001 (MN L A T E X style file v1.4) Prominence support in potential field configurations
 

Summary:  system of AB Doradus by Robinson & Collier Cameron (1986), the same phenomenon has been observed to be al... such as AB Dor and PZ Tel, the field must show significant departures from a simple dipole to distances... derived from a Zeeman­Doppler image of AB Dor yields sufficient field complexity at ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
57 Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 22 April 2011 (MN LATEX style file v2.2) Explanation of the Helium-3 problem
 

Summary:  Doradus in the Large Magellanic Cloud. It has been carefully studied recently (Lopez et al 2008... ). In addition to a large ionized gas mass 8 · 105 M (Kennicutt 1984), the 30 Doradus nebula also has 106 M... : CO in the magellanic clouds - VII. 30 Doradus and its southern HII regions. Astronomy

  

Source: Gibson, Carl H. - Scripps Institution of Oceanography, Center for Astrophysics and Space Sciences, University of California at San Diego

 

Collection: Engineering ; Geosciences

 
58 BOSTON UNIVERSITY GRADUATE SCHOOL OF ARTS AND SCIENCES
 

Summary:  studies of PDRs (e.g., Tielens & Hollenbach 1985a,b) considered the e#11;ects on the ISM of the strong UV... Doradus). In fact, the galaxy-wide [C II]/CO intensity ratio for the LMC is found to be #24; 18 times... and one of the brightest CO (J = 1 ! 0) peaks in the LMC, and 30 Doradus, the brightest H II region

  

Source: Bolatto, Alberto - Department of Astronomy, University of Maryland at College Park

 

Collection: Physics

 
59 prsente par Gilles Ferrand
 

Summary:  -wavelength image of the 30 Doradus superbubble. . . . . . 178 9.2 The Local Bubble... Doradus C. . . . . . . . 182 9.6 X-ray emission from the superbubble NGC 6334. . . . . . . . . . 183 9

  

Source: Ecole Polytechnique, Centre de mathématiques

 

Collection: Mathematics

 
60 The PAH emission spectra of Large Magellanic Cloud H II regions
 

Summary:  and even within 30 Doradus. The LMC spectra have been compared with ISO-SWS spectra from Galactic H II... ­ SMC) is present. Furthermore, within the LMC observations, a clear distinction between 30 Doradus... and non-30 Doradus pointings is found. We discuss the variations in the relative strength of the PAH

  

Source: Groningen, Rijksuniversiteit - Centre for Ecological and Evolutionary Studies, Department of Marine Benthic Ecology and Evolution,

 

Collection: Biology and Medicine ; Environmental Sciences and Ecology


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61 arXiv:astroph/0111050 Mon. Not. R. Astron. Soc. 000, 000{000 (0000) Printed 5 November 2001 (MN L A T E X style le v2.2)
 

Summary:  of densely-sampled, high signal-to-noise echelle spectra of AB Doradus spanning several stellar rotations... - sis to pairs of surface images of the rapidly rotating K dwarf AB Doradus secured several days apart... of high S:N line pro#12;les. Section 2 presents a re-analysis of archival echelle spectra of ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
62 Stellar differential rotation from direct star-spot tracking A. Collier Cameron,1P
 

Summary:  echelle spectra of AB Doradus spanning several stellar rotations in 1996 December. Using spectral... -by-latitude cross-correlation analysis to pairs of surface images of the rapidly rotating K dwarf AB Doradus secured... echelle spectra of AB Doradus observed in 1996 ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
63 RIJKSUNIVERSITEIT GRONINGEN Polycyclic Aromatic Hydrocarbons and dust
 

Summary:  echelle spectra of AB Doradus spanning several stellar rotations in 1996 December. Using spectral... -by-latitude cross-correlation analysis to pairs of surface images of the rapidly rotating K dwarf AB Doradus secured... echelle spectra of AB Doradus observed in 1996 ...

  

Source: Groningen, Rijksuniversiteit - Centre for Ecological and Evolutionary Studies, Department of Marine Benthic Ecology and Evolution,

 

Collection: Biology and Medicine ; Environmental Sciences and Ecology

 
64 Mon. Not. R. Astron. Soc. 378, 12291236 (2007) doi:10.1111/j.1365-2966.2007.11717.x Very high contrast integral field spectroscopy of AB Doradus C
 

Summary:  contrast integral field spectroscopy of AB Doradus C: 9-mag contrast at 0.2 arcsec without a coronagraph... the technique to extract a very high signal-to-noise ratio H- and K-band spectrum of AB Doradus (AB Dor) C... ­ binaries: close ­ stars: individual: AB ...

  

Source: Steward Observatory, Center for Astronomical Adaptive Optics

 

Collection: Physics

 
65 PizzaNacht: Sternentstehung
 

Summary:  Hintergrund ab. Jedes Bild ist 750 AU x 750 AU groß. #12;Ralf Klessen: 30.11.2005 Pillars of God (im... ) IC 1396 (4 Myr) einmassereicherStern #12;Ralf Klessen: 30.11.2005 30 Doradus Region in der Großen

  

Source: Klessen,Ralf - Zentrum für Astronomie, Universität Heidelberg

 

Collection: Physics

 
66 Mon. Not. R. Astron. Soc. 000, 000--000 (1997) Differential rotation and magnetic polarity patterns on
 

Summary:  on AB Doradus ? J.­F. Donati 1 and A. Collier Cameron 2 1 Laboratoire d'Astrophysique, Observatoire Midi... in steady decrease since 1988, our result implies that cool features have moved equatorward on average on AB... . 1 INTRODUCTION The very active southern K0 dwarf AB ...

  

Source: Donati, Jean-François - Observatoire Midi-Pyrénées

 

Collection: Physics

 
67 Astron Astrophys Rev (2007) 14:217360 DOI 10.1007/s00159-007-0007-0
 

Summary:  mentioned above, other classical pulsators exist along the main sequence such as, e.g. the Doradus stars

  

Source: Monteiro, Mário João - Centre for Astrophysics, University of Porto

 

Collection: Physics

 
68 Star and planet formation in young stellar clusters Die meisten Sterne in unserer Milchstrae wer-
 

Summary:  -Haufen im Orion und den 30 Doradus Haufen in der Großen Magellan'schen Wolke, wobei wir uns in erster Linie... Trapezium Cluster in the infrared J,H, and K bands with the VLT (ISAAC) · Direct imaging of the 30 Doradus... Doradus clus- ter are located at 500 pc and 50 kpc distance, respec- tively. In order to derive

  

Source: Astrophysikalisches Institut Potsdam

 

Collection: Physics

 
69 Jorge L. Pineda Curriculum Vitae
 

Summary:  W¨urzburg, Germany Talk: Large Scale Mapping of Molecular Gas in the Vicinity of 30 Doradus... in the Vicinity of 30 Doradus in the Large Magellanic Cloud. Annual Meeting of the Astronomische Gesellschaft (AG... , T., [6 authors], Pineda, J.L., [5 authors] ApJ, 696, 370 The Molecular Ridge Close to 30 Doradus

  

Source: Waliser, Duane E. - Water and Carbon Cycles Group, Jet Propulsion Laboratory

 

Collection: Geosciences

 
70 THE ASTROPHYSICAL JOURNAL, 541:720727, 2000 October 1 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
 

Summary:  to the 30 Doradus Nebula. The large number of shells and networks of shells in 30 Doradus have been identi... , however, that (unlike R136 in 30 Doradus) the ionizing cluster in NGC 604 is not cen- trally concentrated... following a concave curvature. The emission increases once again as one moves toward the ...

  

Source: Muñoz-Tuñón, Casiana - Instituto de Astrofísica de Canarias

 

Collection: Physics

 
71 THE TOPHAT EXPERIMENT: A BALLOON-BORNE INSTRUMENT FOR MAPPING MILLIMETER AND SUBMILLIMETER EMISSION
 

Summary:  , the center of the beam rotation would move in right ascension while remaining at approximately constant dec... , the main feed horn, was re- stricted to move less than $1 mm with respect to the primary mirror... for the thermistor readout. The in-band ab- sorption of the disk was enhanced by placing a backshort ap- proximately

  

Source: Aguirre, James E. - Department of Physics and Astronomy, University of Pennsylvania; Timbie, Peter - Department of Physics, University of Wisconsin at Madison

 

Collection: Physics

 
72 Draft: to appear in Optics Express Fainter and closer: finding planets by symmetry breaking
 

Summary:  . Clarke and L. M. Close, "Very high contrast integral field spectroscopy of AB Doradus C: 9-mag contrast... axis will rotate the distorted Airy pattern and move the speckles in the image plane. Since the images... of the star and planet will not move, the location of the planet will be revealed at different ...

  

Source: Ribak, Erez - Physics Department, Technion, Israel Institute of Technology

 

Collection: Physics

 
73 University of Maryland Department of Astronomy
 

Summary:  with wind infall. Such disks could ab- sorb a large amount of infalling material without a large radii thus... . Pallavicini Arcetri used simultaneous EUVE and ASCA observations to study the corona of the active K dwarf AB... Doradus. They found the surprising result that the abundance of Fe and sev- eral other heavy elements

  

Source: Berkeley Illinois Maryland Association (BIMA)

 

Collection: Physics

 
74 DEPARTMENT OF PHYSICS & ASTRONOMY College of Science
 

Summary:  .15 Duncan Wright Results from a campaign on two gamma Doradus variables 4.15 ­ 4.30 Ewan Orr Category Theory... move across the tropopause from either the troposphere to the stratosphere, or vice versa... and with research from overseas. * * * * * Results from a campaign on two gamma Doradus variables Duncan Wright I

  

Source: Hickman, Mark - Department of Mathematics and Statistics, University of Canterbury

 

Collection: Mathematics

 
75 DEPARTMENT OF PHYSICS & ASTRONOMY College of Science
 

Summary:  of gamma Doradus type candidate stars are currently being used to test these tools. Why I am enthused about... is not moving during the procedure the subtracted image provides details of the vessel anatomy. The subtracted... image is not clear if the patient moves between the images. The study purpose to improve image quality

  

Source: Hickman, Mark - Department of Mathematics and Statistics, University of Canterbury

 

Collection: Mathematics

 
76 WolfRayet stars as gammaray burst progenitors N. Langer a A.J. van Marle a S.C. Yoon b
 

Summary:  shows the formation and evolution of distinct ab­ sorption component, at various radial velocities... ­Taylor instabilities before the collision. After the collision the remnants of the two shells move outward together... for the intermediate velocity ab­ sorption components in the afterglow spectra of GRB 021004, the conclu­ ...

  

Source: Langer, Norbert - Sterrenkundig Instituut, Universiteit Utrecht

 

Collection: Physics

 
77 Mon. Not. R. Astron. Soc. 411, L41L45 (2011) doi:10.1111/j.1745-3933.2010.00988.x Tails of the unexpected: the interaction of an isothermal shell with a cloud
 

Summary:  ablated or stripped from the cloud. The part of the shell adjacent to the cloud moves in the lateral... diminishes as the shell moves further downstream, and the focusing becomes more gradual. A 3D simulation... simulation at t = 0.806 tcc. The shell is moving in the + x direction, and there is reflection symmetry about

  

Source: Pittard, Julian - Department of Physics and Astronomy, University of Leeds

 

Collection: Physics

 
78 ACCEPTED FOR PUBLICATION IN The Astrophysical Journal Preprint typeset using LATEX style emulateapj v. 11/12/01
 

Summary:  magnitudes are in AB system with the fol- lowing zero points: 25.87 (F475W), 26.36 (F606W) and 25.86 (F814W... AB magnitudes of F475W (g) = 21.07, F606W (V) = 21.12, F814W (I) = 22.30. With an abso- lute... A1-A2 (De Marchi et al. 1997). In contrast to the case of 30 Doradus Nebula, which has a very large

  

Source: Johns Hopkins University, Department of Physics and Astonomy, Advanced Camera for Surveys Project

 

Collection: Physics

 
79 Mergers, Interactions, and The Fueling of Starbursts
 

Summary:  to orbital decay and eventual merging. The gas is compressed, dissipates and moves inward, stimulating... activity has historically been defined by some ab­ solute quantity such as IR luminosity, it would... ­ph/9612117) 38. Elmegreen, B. 1994, in ``Violent Star Formation from 30 Doradus to QSOs'', ed. G. Tenorio

  

Source: Hibbard, John - National Radio Astronomy Observatory

 

Collection: Physics

 
80 A&A 428, 209--214 (2004) DOI: 10.1051/00046361:20041266
 

Summary:  di#erences and applied it to # Scuti and # Doradus variables. This method is appropriate for stars... , wavelength region, angles and a specified list of atomic ab­ sorption lines. Specific intensities (I #µ... ) and # = 1 modes do not change significantly, but the ratios for higher order (# > 1) modes move towards

  

Source: Armagh Observatory

 

Collection: Physics


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81 A&A 428, 209214 (2004) DOI: 10.1051/0004-6361:20041266
 

Summary:  differences and applied it to Scuti and Doradus variables. This method is appropriate for stars in which... intensities for a given model atmosphere, wavelength region, angles and a specified list of atomic ab... ) and = 1 modes do not change significantly, but the ratios for higher order ( > 1) modes move towards

  

Source: Armagh Observatory

 

Collection: Physics

 
82 E.S. Phinney, Ay 126, Jan 5 2009 Overview of the Interstellar Medium
 

Summary:  ). Notice redder as move left, farther from Antares, as remaining transmitted light becomes redder. Center... . More recent Chandra results on QSO z=0 abs: Yao et al 2008 ApJ 672, L21 OVII, OVIII, Ne IX K lines... (HII) green: R band 30 Doradus star forming region in LMC #12;E.S. Phinney, Ay 126, Jan 5 2009

  

Source: Phinney, E. Sterl - Division of Physics, Mathematics and Astronomy, California Institute of Technology

 

Collection: Physics

 
83 A&A 428, 209214 (2004) DOI: 10.1051/0004-6361:20041266
 

Summary:  differences and applied it to Scuti and Doradus variables. This method is appropriate for stars in which... intensities for a given model atmosphere, wavelength region, angles and a specified list of atomic ab... ) and = 1 modes do not change significantly, but the ratios for higher order ( > 1) modes move towards

  

Source: Townsend, Richard - Department of Astronomy, University of Wisconsin at Madison

 

Collection: Physics

 
84 Jahresbericht 2009 Mitteilungen der Astronomischen Gesellschaft 93 (2010), 769804 Institut fr Astronomie der Universitt Wien
 

Summary:  ://www.astro.univie.ac.at/ 1 Personal und Ausstattung 1.1 Personalstand Professoren: M. Breger [-51820] bis 30.9., ab dann... emeritiert (bis 30.9. Vizedekan), G. Hensler [-51895] (Institutsleiter bis 30.9., ab 1.10. Vizedekan) Ao... ] (Institutsleiter ab 1.10.), Ass. Prof. J. Hron [51855], Ao. Prof. M.J. Stift [51835], Univ. Doz. ...

  

Source: Astrophysikalisches Institut Potsdam

 

Collection: Physics

 
85 Massive star forming regions from the local Universe to high redshift \Lambda
 

Summary:  massive than previously thought (Kn¨odlseder 2000). In the LMC, the giant H ii region 30 Doradus and it... in the greater 30 Doradus region (from Walborn 1991) Linear Angular 52.5 kpc 1 Mpc 10 Mpc LMC 5 kpc 5 ffi 15' 1... , supershells due to stellar winds and supernovae. Figure 1: Composite image of 30 Doradus showing the ...

  

Source: Schaerer, Daniel - Laboratoire d'Astrophysique de Toulouse, CNRS

 

Collection: Physics

 
86 A&A 470, 941955 (2007) DOI: 10.1051/0004-6361:20065261
 

Summary:  (partly) removing the fringe/ripple pattern it simultaneously re- moves most telluric lines as well... studies show that the relative, though not the ab- solute, depletion levels of heavy elements are constant

  

Source: NASA Ames Research Center, Astrochemistry Laboratory

 

Collection: Physics

 
87 THE ASTROPHYSICAL JOURNAL, 560:934936, 2001 October 20 ( 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
 

Summary:  or S Doradus variables) on the Hertzsprung-Russell (H-R) diagram. The hotter half, 7000È10,000 K, is a nearly... begins moving to the blue. The minimum mass-loss rate needed, however, is close to 10~2 yr~1.M... covered in the same intervals (de Jager & Nieuwenhuijzen 1997). Variable A in M33 seems to have moved just

  

Source: Fridlind, Ann - Earth Science Division, NASA Ames Research Center

 

Collection: Environmental Sciences and Ecology

 
88 Curriculum Vitae : Florian Breuer July 18, 2011 Born: 19 February 1977 in Vienna, Austria.
 

Summary:  Alwis, H. Haupt, "Discovery and analysis of gamma doradus type pulsations in the F0 IV star HR 2740 QW... ." Trans. Amer. Math. Soc., 359 (2007): 1351­1374. 14. F. Breuer, E.C. L¨otter, A.B. van der Merwe, "Ducci

  

Source: Breuer, Florian - Mathematics Department, University of Stellenbosch

 

Collection: Mathematics

 
89 Living Rev. Solar Phys., 2, (2005), 8 http://www.livingreviews.org/lrsp-2005-8
 

Summary:  - type stars was also revealed (Radick et al., 1982, 1983a,b). The solar variations, which never exceed... ). This "bump" moves across the profile, as the star rotates, with the velocity amplitude depending on the spot... line) and with a spot moving across the disk as the star rotates (solid line). See also animation

  

Source: Berdyugina, Svetlana - Kiepenheuer Institut für Sonnenphysik

 

Collection: Physics

 
90 39THE FOURTH PARADIGM EARTH AND ENVIRONMENT
 

Summary:  Wide Telescope view of the 30 Doradus region near the Large Magellanic Cloud. Image courtesy of the National... to move seamlessly back and forth between, for example, spectral line observations of some sources at some

  

Source: Narasayya, Vivek - Data Management, Exploration and Mining Group, Microsoft Research

 

Collection: Computer Technologies and Information Sciences

 
91 THE MISSING LUMINOUS BLUE VARIABLES AND THE BISTABILITY Nathan Smith 1
 

Summary:  LBVs on the S Doradus instability strip at luminosities between log(L=L#12; )' 5.6 and 5.8. The upper... boundary, interestingly, is also where the temperature-dependent S Doradus instability strip intersects... between outbursts. In qui- escence, LBVs generally reside along the S Doradus instability strip, shown

  

Source: Vink, Jorick - School of Physical and Geophysical Sciences, Astrophysics Group, Keele University

 

Collection: Physics

 
92 THE MESSENGER No. 13-June 1978
 

Summary:  to study the tiny planets and to learn more about their physical properties. Although moving in very... trail of a minor planet. Dur- ing the 1'/2-hour exposure, the small planet had moved about 1... of motion, almost due north. This normally means that either the planet is moving in a rather eccentric

  

Source: Liske, Jochen - European Southern Observatory

 

Collection: Physics

 
93 Joe Eggen Page 1 4/18/2008 A Report on the Theory of Pulsating Stars
 

Summary:  of the star's surface move inwards while other parts move outwards. Whereas one number, the order... . Examples of nonradial pulsators include pulsating white dwarfs, Gamma Doradus stars, Beta Cepheids... is an opacitydriven phenomenon. As one moves inward from the surface through the atmosphere of a ...

  

Source: Wiita, Paul J. - Department of Physics and Astronomy, Georgia State University

 

Collection: Physics

 
94 STUDY OF STAR FORMATION REGIONS WITH MOLECULAR HYDROGEN EMISSION LINES
 

Summary:  mode and the reference source, we can see moving interference fringes on the screen. If the two mirrors

  

Source: Pak, Soojong - Department of Astronomy and Space Science, Kyung Hee University

 

Collection: Physics

 
95 The Astrophysical Journal Supplement Series, 194:1 (28pp), 2011 May doi:10.1088/0067-0049/194/1/1 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
 

Summary:  that there are multiple generations of massive stellar clusters in 30 Doradus, the Local Group's most powerful GEHR... ; the Carina complex might represent a miniaturized version of 30 Doradus--a smaller sample in both space... cluster R136 in 30 Doradus (Townsley et al. 2006a, 2006b), this observation yielded over 1600 X-ray ...

  

Source: Pittard, Julian - Department of Physics and Astronomy, University of Leeds

 

Collection: Physics

 
96 The Nature and Evolution of Disks Around Hot Stars ASP Conference Series, Vol. TBD, 2005
 

Summary:  to the same line seen in the MEG spectrum of the active young M dwarf, AB Doradus. An absolutely narrow model... the disks of these stars is already moving at 0.95 vcrit. And it also demonstrates how even straightforward... material as the photons work their way through the disk (Wood & Bjorkman 1995; Wood et al. ...

  

Source: Cohen, David - Department of Physics and Astronomy, Swarthmore College

 

Collection: Plasma Physics and Fusion ; Physics

 
97 A&A manuscript no. (will be inserted by hand later)
 

Summary:  in late­type rapid rotators The case of HK Aquarii & AB Doradus G.H.J. van den Oord 1 , M.T. Eibe 2... .03.3; 08.09.2; HK Aqr; AB Dor; 08.12.1; 13.21.5 ASTRONOMY AND ASTROPHYSICS 26.2.1997 Prominence­like clouds... ­ ism to the case of neutral hydrogen clouds in the rapidly rotating late­type stars, HK Aqr and ...

  

Source: Armagh Observatory

 

Collection: Physics

 
98 UNVEILING THE LOW-FREQUENCY UNIVERSE
 

Summary:  ). The Astrophysi- cal Journal, Volume 739, Issue 2, article id. 83 (2011). http:// adsabs.harvard.edu/abs/2011Ap... .06.033 STar formaTion in 30 doraduS De Marchi, G. et al. (including Rogier Windhorst). The Astro- physical... Journal, Volume 739, Issue 1, article id. 27 (2011). http://adsabs.harvard.edu/abs/2011ApJ...739...27D

  

Source: Shumway, John - Department of Physics and Astronomy, Arizona State University

 

Collection: Physics ; Materials Science

 
99 Astrophysical Journal, Vol. 551, p 1099, April 10 2001 On the formation of polar spots in Sunlike stars
 

Summary:  of AB Doradus (Donati et al, 1999), perhaps somehow associated with the sheared filament configuration... been reported on young, rapidly rotating main­sequence stars, such as on AB Dor (K0 V; e.g., Donati et... latitudes, and that then move poleward in what appears to be a meridional flow at 6­30 m s ...

  

Source: Schrijver, Karel - Solar and Astrophysics Laboratory, Lockheed Martin

 

Collection: Physics

 
100 THE ASTROPHYSICAL JOURNAL, 551:10991106, 2001 April 20 ( 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
 

Summary:  in this polarity pattern could cause what appears to be a ring of azimuthal Ðelds encircling the pole of AB Doradus... been reported on young, rapidly rotating main- sequence stars, such as AB Dor (K0 V; see, e.g., Donati... rate. They claim to observe spots that form at low latitudes and then move poleward ...

  

Source: Schrijver, Karel - Solar and Astrophysics Laboratory, Lockheed Martin

 

Collection: Physics


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