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

• A strong flare in the K dwarf LQ Hya Departamento de Astrof'isica, Facultad de F'isicas,
• A. Klutsch1, D. Montes1, P. Guillout2, A. Frasca3, F.-X. Pineau2, N. Grosso2, E. Marilli3, J. Lpez-Santiago1 1 Universidad Complutense de Madrid, Dpt. de Astrofsica, Facultad C.C. Fsicas, Madrid, Spain, E-mail : klutsch@astrax.fis.ucm.es
• R.M. Martnez-Arniz1, J. Maldonado2,D. Montes1, C. Eiroa2, B. Montesinos3,5, I. Ribas4, E. Solano3 1 Universidad Complutense de Madrid, Dpt. de Astrofsica, Facultad C.C. Fsicas, Madrid, Spain,
• Spectroscopic surveys of possible late-type stars members
• Stellar Kinematic Groups are kinematical coherent groups of stars which may share a common origin. These groups spread through The Galaxy over time due to tidal effects caused by galactic rotation and disk heating, however the chemical information survive
• Program Stars and Stellar Parameters Table. 1: Stellar parameters of the observed stars: spectral type (SpT), vsin(i) and photometric period
• The chromospheric activity of weak line T Tauri stars: simultaneous Hff and Ca ii H & K observations
• Chromospherically active binaries members of young stellar kinematic groups
• A&A 389, 524--536 (2002) DOI: 10.1051/00046361:20020644
• RESPUESTA DE DIFERENTES LNEAS DE EMISIN DEL RANGO PTICO A VARIAS FULGURACIONES OBSERVADAS
• Spectroscopic analysis of the extremely active binaries BK Psc and XX Tri
• CHROMOSPHERIC ACTIVITY OF WEAKLINED T TAURI STARS
• A&A manuscript no. (will be inserted by hand later)
• The broad components in the Hff line of very active stars: chromospheric microflaring?
• A&A manuscript no. (will be inserted by hand later)
• Spectroscopy follow up of planet-bearing stars M.C. Galvez1,2
• Excess Hfi emission in five chromospherically active binaries
• Detection of Li i enhancement during a longduration flare in the recenltly discovered Xray/EUV selected, chromospher
• Identification of isolated post T Tauri stars in the solar neighborhood
• Latetype stars members of young stellar kinematic groups D. Montes 1 , A. Latorre 1 , M.J. Fern'andezFigueroa 1
• The 11 th Cool Stars, Stellar Systems and the Sun ASP Conference Series, Vol. 223, 2001
• THE ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 123:283293, 1999 July 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• Late-type members of young stellar kinematic groups I. Single stars D. Montes,P
• The nearest young moving groups J. Lopez-Santiago1,2
• The First Extrasolar Planet Discovered with a New Generation High Throughput Doppler Instrument
• Multiwavelength optical observations of two chromospherically active binary systems: V789 Mon and GZ Leo
• Astronomy & Astrophysics manuscript no. catrass10dec2008rev c ESO 2009 March 24, 2009
• arXiv:1002.4391v1[astro-ph.SR]23Feb2010 Astronomy & Astrophysics manuscript no. activityrmafinal c ESO 2010
• D. Montes1, I. Crespo-Chacn1, M.J. Fernndez-Figueroa1, J. Lpez-Santiago1, D. Garca Alvarez2, 3, B.H. Foing4
• Stars as Suns: Activity, Evolution, and Planets IAU Symposium, Vol. 219, 2004
• En esta contribucin se describe la exploracin espectroscpica de alta resolucin que estamos llevando a cabo para estrellas aisladas de los ltimos tipos, identificadas en nuestros anteriores estudios como posibles miembros de grupos cinemticos jvenes: (Asoc
• During the last years (1999 -2004), our group has been studying the spectroscopic properties of a large sample of stars members of the
• FLARE STARS AMONG K DWARFS MEMBERS OF YOUNG STELLAR KINEMATIC GROUPS D. Montes, J. Lopez-Santiago, I. Crespo-Chacon, and M. J. Fernandez-Figueroa
• A STUDY ON THE FLUX-FLUX AND ACTIVITY-ROTATION RELATIONSHIPS FOR LATE-TYPE STARS MEMBERS OF YOUNG STELLAR KINEMATIC GROUPS
• HIGH TEMPORAL RESOLUTION SPECTROSCOPIC OBSERVATIONS OF UV CET TYPE FLARE STARS
• High Resolution Spectroscopy of Recently Discovered Chromospherically Active Binary Stars
• From microflares to strong and long-duration flares D. Montes, J. Lopez-Santiago, I. Crespo-Chacon, M.J. Fernandez Figueroa
• Chromospheric activity variations in late-type stars members of young stellar kinematic groups
• Fig. 2: a) Spectra of PW And in a maximum and a minimum of emission; b) Variation in
• D. Montes, M.C. Glvez, M.J. Fernndez-Figueroa, I. Crespo-Chacn, Universidad Complutense de Madrid, Dpt. de Astrofsica,
• Highlights of Astronomy, Volume 14 XXVIth IAU General Assembly, August 2006
• Cool stars in the solar neighborhood. Preparatory activities for the Darwin mission
• High resolution spectra of cool stars in the Virtual Observatory. Criteria for spectral
• D. Montes1, J. Lpez-Santiago1,2, I. Crespo-Chacn1, R.M. Martnez-Arniz1, J. Maldonado1,3
• Active regions in a sample of late-type rotator stars: spectroscopic analysis
• Spectroscopic properties of UVSpectroscopic properties of UV CetiCeti--type Starstype Stars I. Crespo-Chacn1, J. Lpez -Santiago2, D. Montes1, M. J. Fernndez-Figueroa1
• D. Montes1, UCM cool stars group2, & Spanish Virtual Observatory3 1 Universidad Complutense de Madrid, Dpt. de Astrofsica, Facultad C.C. Fsicas, Madrid, Spain, dmg@astrax.fis.ucm.es,
• Selection from the lithium (Age) Spectra of some Pic Moving Group members
• Spectroscopic Studies of Nearby Cool Stars: The DUNES Sample
• I. Crespo-Chacn1, J. Lpez-Santiago1, D. Montes1, M. J. Fernndez-Figueroa1, G. Micela2, F. Reale2,3, D. Garca-lvarez4,5,6, M. Caramazza2,3, I. Pillitteri3.
• arXiv:0810.2030v1[astro-ph]11Oct2008 Preliminary results on a Virtual Observatory
• Selection from the Lithium (Age) Spectra of some Pic Moving Group members
• Post T Tauri stars in the solar neighborhood: isolated or members of young associations and
• High resolution spectroscopic characterization of the FGK stars in the Solar neighbourhood
• We present the most recent results of our ongoing long-term high resolution spectroscopic study of nearby (d < 25 pc) FGK stars, which aim is to characterize the local properties of the Galaxy, in
• Acknowledgments: This work was supported by Universidad Complutense de Madrid (UCM), the Spanish Ministerio de Ciencia e Innovacin (MICINN) under grant AYA2008-00695, and "The Comunidad de Madrid" under PRICIT project S-0505/ESP-0237 (ASTROCAM)
• A. Klutsch1,2, P. Guillout2 , R. Freire Ferrero2, A. Frasca3, E. Marilli3 , and D. Montes1 1 Universidad Complutense de Madrid,Dpt. de Astrofsica, Facultad C.C. Fsicas, Madrid, Spain, E-mail : klutsch@astrax.fis.ucm.es
• Discovery of co-moving young stars in Cepheus P. Guillout1 ,
• Pathways Towards Habitable Planets ASP Conference Series, Vol. 430, 2010
• J. A. Caballeroa, A. Quirrenbachb, P. Amadoc, H. Mandeld, I. Ribase, A. Reinersf and the CARMENES Consortium1,2,3,4,5,6,7,8,9
• Pathways Towards Habitable Planets ASP Conference Series, Vol. 430, 2010
• Acknowledgments: This work was supported by Universidad Complutense de Madrid (UCM), the Spanish Ministerio de Ciencia e Innovacin
• High resolution spectroscopy of late-type stars: understanding the chromospheric activity paradigm,
• **Volume Title** ASP Conference Series, Vol. **Volume Number**
• Stellar kinematic groups (stellar streams, moving groups, and associations)
• Stellar Kinematic Groups are kinematical coherent groups of stars which may share a common origin. These groups spread through The Galaxy over time due to tidal effects caused by galactic rotation and disk heating, however the chemical information survive
• SWG DRC Acronym MOS R (/) N of targets N of nights MW DRC1 2E5 20,000 (MOS) 200,000 stars 30
• Agradecimientos: Estas actividades se han desarrollado gracias al apoyo y financiacin recibidos por la Universidad Complutense de
• Universidad Complutense de Madrid Facultad de CC. Fisicas
• FLARE STARS AMONG K DWARFS MEMBERS OF YOUNG STELLAR KINEMATIC GROUPS D. Montes, J. Lopez-Santiago, I. Crespo-Chacon, and M.J. Fernandez-Figueroa
• VO-COMPLIANT LIBRARIES OF HIGH RESOLUTION SPECTRA OF COOL STARS David Montes1,4
• A&A 379, 976--991 (2001) DOI: 10.1051/00046361:20011385
• Mon. Not. R. Astron. Soc. 000, 1--?? (1998) Printed 27 November 1998 (MN L a T E X style file v1.4) Optical and UV observations of a strong flare in the young,
• David Montes, Elisa De Castro, Jaime Zamorano, Jess Gallego El Departamento de Astrofsica y C.C. de la Atmsfera de la Universidad Complutense de Madrid (UCM) ha dedicado
• Mining the sky for isolated very young starsMining the sky for isolated very young starsMining the sky for isolated very young stars P. GuilloutP. Guillout11,,
• A&A 491, 515523 (2008) DOI: 10.1051/0004-6361:200810616
• Astronomy & Astrophysics manuscript no. MS3636 September 3, 2003 (DOI: will be inserted by hand later)
• FR Cnc Nature Revisited M.C. Galvez, A. Golovin, M. Hernan-Obispo, E. Pavlenko, M. Andreev, D.
• D. Montes, J. Lpez-Santiago, I. Crespo-Chacn, M.J. Fernndez-Figueroa, Universidad Complutense de Madrid, Dpt. de Astrofsica, Facultad de Ciencias Fsicas, E-28040 Madrid, Spain
• Stellar Coronae in the Chandra and XMMNewton Era ASP Conference Series, Vol. TBD, 2001
• Mon. Not. R. Astron. Soc. 000, 1{?? (2001) Printed 28 June 2001 (MN L a T E X style le v1.4) Late-type stars members of young stellar kinematic groups
• The 11 th Cool Stars, Stellar Systems and the Sun ASP Conference Series, Vol. 223, 2001
• Highlights of Spanish Astrophysics VI, Proceedings of the IX Scientific Meeting of the Spanish Astronomical Society held on September 13 -17, 2010, in Madrid, Spain. M. R. Zapatero Osorio et al. (eds.)
• During our detailed study of the kinematics of the known exoplanets-hots stars (Montes et al. 2010; Caballero et al. 2010) we have identified possible members of the classical moving groups with ages between 10 and 600 Myr (e.g. Local Association, Castor,
• !!Moving groups (MGs): During the last 20 years, many studies (see, e.g., Jeffries 1995; Montes et al. 2001) have shown that a fraction of X-ray active and lithium-rich stars are
• Context. Young exoplanetary systems with ages 600 Ma (i.e. Hyades-like or younger) can provide constraints on the time scale and mechanism of planet
• HIGH RESOLUTION SPECTROSCOPIC SURVEY OF SINGLE LATE-TYPE STARS
• Multiwavelength optical observations of the chromospherically ac tive binary system OU Gem
• Highlights of Spanish Astrophysics VI, Proceedings of the IX Scientific Meeting of the Spanish Astronomical Society held on September 13 -17, 2010, in Madrid, Spain. M. R. Zapatero Osorio et al. (eds.)
• The X-ray/EUV selected binary 2RE J0933+624 (FF UMa): orbital solution and chromospheric activity
• III) New young stars in the CO Cepheus void !!Selecting an appropriate sample of targets is the major difficulty for searching other co-moving young stars in this sky area. We
• Astronomy & Astrophysics manuscript no. (will be inserted by hand later)
• Astron. Astrophys. 330, 155--168 (1998) ASTRONOMY ASTROPHYSICS
• Highlights of Spanish Astrophysics VI, Proceedings of the IX Scientific Meeting of the Spanish Astronomical Society held on September 13 -17, 2010, in Madrid, Spain. M. R. Zapatero Osorio et al. (eds.)
• MUSICOS 1998: Observations of Rotational Modulation and Flares on the RS CVn Binary HR1099
• David Montes, Elisa De Castro, Jaime Zamorano, Jess Gallego La Universidad Complutense de Madrid (UCM) tiene gran tradicin en las enseanzas de Astrofsica. Desde 1972 en
• Astronomy & Astrophysics manuscript no. skgsurveycatalogfv c ESO 2010 February 9, 2010
• J. Maldonado1,2, R.M. Martnez-Arniz1, D. Montes1, C. Eiroa2, B. Montesinos3,4, I. Ribas5, E. Solano4
• IAU Symp. 240: Binary Stars as Critical Tools & Tests in Con-temporary Astrophysics
• Multiwavelength optical observations of the chromospherically active binary system MS Ser
• Fig.4. Spatial distribution of stellar X-ray sources located
• Departamento de Astrofsica, Facultad de Ciencias Fsicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain Collaborators (alphabetical order): Crespo-Chacn I., De Castro E., Daz C., Gallego J., Glvez M.C.,
• A&A manuscript no. (will be inserted by hand later)
• Young stellar kinematic groups and their relation with young open clusters, star forming regions and the Gould Belt
• Astronomy & Astrophysics manuscript no. MS3636 September 2, 2003 (DOI: will be inserted by hand later)
• Multiwavelength optical observations of the chromospherically ac tive binary system HU Vir
• The 11 th Cool Stars, Stellar Systems and the Sun ASP Conference Series, Vol. 223, 2001
• Chromospheric activity, lithium and radial velocities of late-type stars members of young stellar kinematic groups
• R.M. Martnez-Arniz1, J. Maldonado1,2, D. Montes1, C. Eiroa2, B. Montesinos3,4, I. Ribas5, E. Solano4 1 Universidad Complutense de Madrid, Dpt. de Astrofsica, Facultad C.C. Fsicas, Madrid, Spain,
• Pathways Towards Habitable Planets ASP Conference Series, Vol. 430, 2010
• Spectroscopic observations (high resolution echelle spectra) of 236 stars were obtained by our team beteween 2005 and 2007 by using the FOCES spectrograph at
• SPECTROSCOPIC MONITORING WITH HIGH TEMPORAL RESOLUTION OF THE
• ASTRONOMY & ASTROPHYSICS OCTOBER II 1997, PAGE 263 SUPPLEMENT SERIES
• High resolution spectra of flare M-dwarfs Crespo-Chacon I., Montes D., Fernandez-Figueroa M.J., Lopez-Santiago J.
• IAU Symp. 240: Binary Stars as Critical Tools & Test in Contem-porary Astrophysics
• The 11 th Cool Stars, Stellar Systems and the Sun ASP Conference Series, Vol. 223, 2001
• Exoplanet host stars in young moving groups: preliminary results
• COOL STARS: CHROMOSPHERIC ACTIVITY, ROTATION, KINEMATIC AND AGE
• MULTIWAVELENGTH OPTICAL OBSERVATIONS OF THREE X RAY/EUV
• Multiwavelength optical observations of three X ray/EUV selected binaries
• LATE-TYPE STELLAR POPULATION OF YOUNG MOVING Departamento de Astrof sica, Facultad de F sicas, Universidad
• High Temporal Resolution Spectroscopic Observations of the Flare Star V1054 Oph
• The X ray/EUV Selected Binary 2RE J0933+624 (FF Uma): Orbital Solution and Chromospheric Activity
• D. Montes1, J. Lpez-Santiago1, M.J. Fernndez-Figueroa1, L.W. Ramsey2 1 Universidad Complutense de Madrid, Dpt. de Astrofsica, Facultad de Ciencias Fsicas, E-28040 Madrid, Spain.
• 1 Universidad Complutense de Madrid, Dpto. de Astrofsica, Fac. C.C. Fsicas, Madrid, Spain, 2 Universidad Autnoma de Madrid, Dpto de Fsica Terica C-XI, Fac. de Ciencias, Madrid, Spain
• D. Montes1, R.M. Martnez-Arniz1, J. Maldonado1,2, J. Roa-Llamazares1, J. Lpez-Santiago1,3, I. Crespo-Chacn1, M.C. Glvez1, E. Solano4
• Stellar Kinematic Groups are kinematical coherent groups of stars which might share a common origin. These groups spread through the Galaxy over time due to tidal effects caused by galactic rotation and disk heating, however the chemical information survi
• Highlights of Spanish Astrophysics VI, Proceedings of the IX Scientific Meeting of the Spanish Astronomical Society held on September 13 -17, 2010, in Madrid, Spain. M. R. Zapatero Osorio et al. (eds.)
• David Montes, Jaime Zamorano, Jess Gallego, Elisa De Castro La Universidad Complutense de Madrid (UCM) tiene gran tradicin en las enseanzas de Astrofsica. Desde 1972 en
• **Volume Title** ASP Conference Series, Vol. **Volume Number**
• ROTATIONAL MODULATION OF THE PHOTOSPHERIC ANDCHROSMOSPHERIC
• LIBRARIES OF HIGH AND MIDRESOLUTION SPECTRA OF F, G, K, AND M FIELD STARS
• Spectroscopic monitoring with high temporal resolution of the flare star AD Leo
• Orbital Period Variation in the Chromospherically Active Binary FF UMa (2RE J0933+624)
• A&A manuscript no. (will be inserted by hand later)
• Astron. Astrophys. 330, 155168 (1998) ASTROPHYSICS
• Chromospheric activity and orbital solution of six new late-type spectroscopic binary systems
• A longduration flare in the Xray/EUV selected chromospherically ac tive binary 2RE J0743+224
• High resolution spectroscopic characterization of the FGK stars in the solar neighbourhood
• Astronomy & Astrophysics manuscript no. 7015galvezfv c ESO 2007 June 25, 2007
• High resolution spectroscopic analysis of cool stars possible members of the AB Doradus
• D. Montes, I. Crespo-Chacn, M.C. Glvez, M.J. Fernndez-Figueroa, Universidad Complutense de Madrid, Dpto. de Astrofsica,
• FR Cnc Nature Revisited M.C. Glvez1, 2 , A. Golovin3, 4, M. Hernn-Obispo2, E. Pavlenko5, M. Andreev6, M., D. Montes2,
• Ins Crespo-Chacn, David Montes, Javier Lpez-Santiago, M Jos Fernndez-Figueroa Departamento de Astrofsica, Facultad de Ciencias Fsicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain
• Astron. Astrophys. 340, L5--L9 (1998) ASTRONOMY ASTROPHYSICS
• HIGH RESOLUTION SPECTROSCOPY OF RECENTLY DISCOVERED CHROMOSPHERICALLY ACTIVE BINARY STARS
• Fig. 15: log FS(Ca II 8542) vs. log Pphot for the stars of the sample. Different symbols are used for
• **Volume Title** ASP Conference Series, Vol. **Volume Number**
• Introduction Kinematic Analysis Age estimates Final membership Summary Spectroscopic properties of nearby
• Astronomy & Astrophysics manuscript no. 3615text March 3, 2006 (DOI: will be inserted by hand later)
• Multiwavelength optical observations of chromospherically active binary systems
• MULTIWAVELENGTH OPTICAL OBSERVATIONS OF CHROMOSPHERICALLY ACTIVE BINARY SYSTEMS
• Chromospherically active binaries members of young open Departamento de Astrof'isica, Facultad de F'isicas, Universidad
• Chromospheric activity of the doublelined spectroscopic binary BF Lyn D. Montes 1 , R. Lachaume 1;2 , M.J. Fern'andezFigueroa 1
• The local association moving group: late-type members and age subgroups
• A&A manuscript no. (will be inserted by hand later)
• Pathways Towards Habitable Planets ASP Conference Series, Vol. 430, 2010
• submitted to The Astrophysical Journal Supplement Series Library of mediumresolution fiber optic echelle spectra of F, G, K, and M field
• Chromospheric activity of ROSAT discovered weaklined T Tauri stars D. Montes 1;2 , L.W. Ramsey 1
• Spectroscopic survey of late-type stars possible members of young moving groups
• Highlights of Spanish Astrophysics VI, Proceedings of the IX Scientific Meeting of the Spanish Astronomical Society held on September 13 -17, 2010, in Madrid, Spain. M. R. Zapatero Osorio et al. (eds.)
• Divulgacion de la Astronomia y Astrofisica en el Observatorio UCM Colaboradores, por orden alfabetico: Crespo-Chacon I., Diaz C., De Castro E.,
• Relationships between physical and observational parameters during flares on
• D. Montes1, J. Lpez-Santiago1,2, I. Crespo-Chacn1, R.M. Martnez-Arniz1, J. Maldonado1,3
• Selection from the Lithium (Age) Spectra of some Pic Moving Group members
• A&A 379, 976991 (2001) DOI: 10.1051/0004-6361:20011385
• We present a detailed study of the kinematics (Galactic space motions U, V , W) of a sample of very low-mass ultracool dwarfs (spectral type later than M7) with radial velocities and proper motions determined in the literature. Spectrophotometric distance
• Stellar Clusters & Associations: A RIA Workshop on Gaia Granada, 23rd -27th May 2011
• Methods. On 2012 Feb 29, the Extrasolar Planets Encyclopaedia (exoplanet.eu) tabulated 699 planet candidates in 558 planetary systems detected by radial velocity (93 multiple planet systems). Of them, over 300 have Hipparcos
• OFERTA DE 2 BECAS FPI PARA EL PROYECTO CARMENES El Proyecto coordinado "Deteccin y estudio de planetas alrededor de estrellas poco