The Pseudocontinuum Bound‐Free Opacity of Hydrogen and Its Importance in Cool White Dwarf Atmospheres
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference17 articles.
1. Temperature dependence of the Lyman αline wings in cool hydrogen-rich white dwarf atmospheres. Application to ZZ Ceti white dwarf spectra
2. Electronic Eigenenergies of the Hydrogen Molecular Ion
3. The Halo White Dwarf WD 0346+246 Revisited
4. The Chemical Evolution of Cool White Dwarfs and the Age of the Local Galactic Disk
5. Synthetic spectra and atmospheric properties of cool DA white dwarfs
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1. NEAR-UV ABSORPTION IN VERY COOL DA WHITE DWARFS;The Astrophysical Journal;2014-07-02
2. Infrared absorption of dense helium and its importance in the atmospheres of cool white dwarfs;Astronomy & Astrophysics;2014-06
3. 11-12 Gyr old white dwarfs 30 pc away;Monthly Notices of the Royal Astronomical Society: Letters;2012-05-04
4. Collision-induced dipoles and polarizabilities of pairs of hydrogen molecules: Ab initio calculations and results from spherical tensor analysis;AIP Conference Proceedings;2012
5. Lyman α wing absorption in cool white dwarf stars;Monthly Notices of the Royal Astronomical Society;2010-11-23
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