The Physics of Pulsating White Dwarf Stars

被引：0
|
作者：
Fontaine, G. [1 ]
Brassard, P. [1 ]
Charpinet, S. [2 ]
Dufour, P. [1 ]
Quirion, P. -O [3 ]
Randall, S. K. [4 ]
Van Grootel, V. [5 ]
机构：
[1] Univ Montreal, Dept Phys, CP 6128, Montreal, PQ H3C 3J7, Canada
[2] Univ Toulouse, CNRS, UPS OMP IRAP, F-31400 Toulouse, France
[3] Agence Spatiale Canadienne, Longueuil, PQ J3Y 8Y9, Canada
[4] European Southern Observ, D-85748 Munich, Germany
[5] Univ Liege, Inst dAstrophys & Geophys, B-B4000 Liege, Belgium
来源：
PROGRESS IN SOLAR/STELLAR PHYSICS WITH HELIO- AND ASTEROSEISMOLOGY | 2012年 / 462卷
基金：
加拿大自然科学与工程研究理事会;
关键词：
DB GAP; HYDROGEN; STATE; EQUATIONS; CATALOG; PLASMAS; HELIUM; MODELS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present a summary of the properties of white dwarf stars, beginning with a brief reminder of their basic characteristics. We continue with a discussion of the spectral types, evolution, and other properties of cooling white dwarfs, with an emphasis on the internal physics. We then introduce the pulsating white dwarfs and provide an updated view of their status. We finally discuss the impact (real and potential) of asteroseismology on our knowledge of degenerate stars.
引用
收藏
页码：477 / +
页数：3
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