A Confirmation of the Optical Spectroscopy Approach: Discovery of Two More Pulsating DA (ZZ Ceti) White Dwarfs-Reference-Cited by-同舟云学术

A Confirmation of the Optical Spectroscopy Approach: Discovery of Two More Pulsating DA (ZZ Ceti) White Dwarfs

Published:2003-07-10 Issue:2 Volume:591 Page:1184-1191
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Fontaine G.,Bergeron P.,Billeres M.,Charpinet S.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/591/i=2/a=1184/pdf

Reference34 articles.

1. A spectroscopically predicted new ZZ Ceti variable - GD 165

2. A spectroscopic determination of the mass distribution of DA white dwarfs

3. New model atmospheres for very cool white dwarfs with mixed H/He and pure He compositions

4. Optical and Ultraviolet Analyses of ZZ Ceti Stars and Study of the Atmospheric Convective Efficiency in DA White Dwarfs

5. Billeres, M. & Fontaine, G. 2003, in Asteroseismology Across the HR Diagram, ed. M. J. Thompson, M. S. Cunha, & M. J. P. F. G. Monteiro (Dordrecht: Kluwer), in press

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