The Composition and Structure of White Dwarf Atmospheres Revealed by Extreme Ultraviolet Spectroscopy
- 1 January 1996
- book chapter
- Published by Springer Nature
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- Non-LTE line-blanketed model atmospheres of hot stars. 1: Hybrid complete linearization/accelerated lambda iteration methodThe Astrophysical Journal, 1995
- Non-LTE line-blanketed model atmospheres of hot stars. 2: Hot, metal-rich white dwarfsThe Astrophysical Journal, 1995
- Detection of episodic mass outflow in the newly discovered hot DO white dwarf RE 0503 - 289Monthly Notices of the Royal Astronomical Society, 1994
- Extreme-ultraviolet spectrophotometry of HD 15638 and HR 8210 (IK Peg)Monthly Notices of the Royal Astronomical Society, 1994
- A spectroscopic analysis of DAO and hot DA white dwarfs: The implications of the prescence of helium and the nature of DAO starsThe Astrophysical Journal, 1994
- Limits on the hydrogen layer mass and consequent helium opacity in hot DA white dwarf atmospheresMonthly Notices of the Royal Astronomical Society, 1994
- The nature of the newly discovered DO white dwarf RE 0503 - 289Monthly Notices of the Royal Astronomical Society, 1994
- ROSAT studies of the composition and structure of DA white dwarf atmospheresMonthly Notices of the Royal Astronomical Society, 1993
- A computer program for calculating non-LTE model stellar atmospheresComputer Physics Communications, 1988
- The luminosity function of DA white dwarfsThe Astrophysical Journal, 1986