
- R. Astron. 337, 1340--1348 (2002) Radiative accelerations on Ne in the atmospheres of late stars
- The A-Star Puzzle Proceedings IAU Symposium No. 224, 2004
- Astronomy & Astrophysics manuscript no. waspAm c ESO 2011 July 1, 2011
- Astron. Astrophys. 333, 665--672 (1998) ASTRONOMY ASTROPHYSICS
- Neon abundances in normal late-B and mercurymanganese stars M. M. Dworetsky 1# and J. Budaj 1,2#
- The A-Star Puzzle Proceedings IAU Symposium No. 224, 2004
- Mon. Not. R. Astron. Soc. 337, 13401348 (2002) Radiative accelerations on Ne in the atmospheres of late B stars
- Neon abundances in normal late-B and mercurymanganese stars M. M. Dworetsky1w
- Astron. Astrophys. 333, 665672 (1998) ASTROPHYSICS
- Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 10 October 2008 (MN LATEX style file v2.2) High Spatial Resolution Galactic 3D Extinction Mapping with
- An Atlas of Stellar Spectra
- REVISED MK SPECTRAL ATLAS FOR STARS EARLIER THAN THE SUN
- Mon. Not. R. Astron. Soc. 000, 124 (2002) Printed 28 July 2009 (MN LATEX style file v2.2) Effects of Dark Matter Substructures on Gravitational
- Modern Physics, Astronomy, and Cosmology Partial Notes, Astronomy Set 2 Galaxies
- Perception, 1996, volume 25, pages 1385-1388 Original Sinn
- Modern Physics, Astronomy, and Cosmology http://www.star.ucl.ac.uk/~idh/1B23
- 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
- Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 26 April 2010 (MN LATEX style file v2.2) Full-sky map of the ISW and Rees-Sciama effect from Gpc
- Online Material Appendix A: Galaxy image and (r) profile catalogue
- Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 28 April 2010 (MN LATEX style file v2.2) Supplementary material
- Full linelist This table lists the lines and equivalent widths measured for AE Her. All wavelengths
- Mon. Not. R. Astron. Soc. 000, 1--21 (2009) Printed 30 March 2009 (MN L A T E X style file v2.2) Orbitally modulated dust formation by the WC7+O5
- REVISED MK SPECTRAL ATLAS FOR STARS EARLIER THAN THE SUN
- An Atlas of Stellar Spectra
- An Atlas of Stellar Spectra
- Abundance analysis of normal and mercurymanganese type lateB stars from
- The abundance tables The abundances are quoted relative to the stellar hydrogen abundance and are listed
- This chapter is divided into three sections. Section 7.1, `Trends', highlights possible links between factors which may govern the emergence of the HgMn phenomenon
- Final comments and conclusions This work has shown that it is possible to obtain highquality abundance deter
- Comparison to the literature The abundance patterns for each star taken from this thesis and from the literature
- Observations and reduction 2.1 Choice of stars
- REVISED MK SPECTRAL ATLAS FOR STARS EARLIER THAN THE SUN
- Metal abundance analysis 5.1 The line abundance
- Abt, H.A., 1979. Astrophys. J., 230, 485 Adelman, S.J., 1973. Astrophys. J., 182 531
- Spectrum analysis and synthesis 3.1 Spectrum analysis
- Introduction 1.1 Overview
- Structure Formation by Fifth Force I: N-Body vs. Linear Simulations Baojiu Li1, 2,
- Mon. Not. R. Astron. Soc. 000, 000000 (0000) Printed 7 August 2008 (MN LATEX style file v2.2) The kinematic footprints of five stellar streams in
- Modern Physics, Astronomy, and Cosmology http://www.star.ucl.ac.uk/~idh/1B23