A Driving Mechanism for the Newly Discovered Class of Pulsating Subdwarf B Stars-Reference-Cited by-同舟云学术

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A Driving Mechanism for the Newly Discovered Class of Pulsating Subdwarf B Stars

Published:1997-07-10 Issue:2 Volume:483 Page:L123-L126
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Charpinet S.,Fontaine G.,Brassard P.,Chayer P.,Rogers F. J.,Iglesias C. A.,Dorman B.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference22 articles.

1. Brassard, P. & Fontaine, G. 1994, in IAU Colloq. 147, The Equation of State in Astrophysics, ed. G. Chabrier & E. Schatzman (Cambridge: Cambridge Univ. Press), 560

2. Brassard, P., Fontaine, G. & Bergeron, P. 1997, in preparation

3. The Potential of Asteroseismology for Hot, Subdwarf B Stars: A New Class of Pulsating Stars?

4. Radiative Levitation in Hot White Dwarfs: Equilibrium Theory

5. Improved Calculations of the Equilibrium Abundances of Heavy Elements Supported by Radiative Levitation in the Atmospheres of Hot DA White Dwarfs

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