A nonadiabatic oscillation study of DB white dwarfs

被引：22

作者：

Gautschy, A ^{[1
]}

Althaus, LG ^{[1
]}

机构：

[1] Natl Univ La Plata, Fac Ciencias Astron & Geofis, RA-1900 La Plata, Argentina

来源：

ASTRONOMY & ASTROPHYSICS | 2002年 / 382卷 / 01期

关键词：

stars : oscillations; stars : white dwarfs; stars : interior;

D O I：

10.1051/0004-6361:20011607

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A self-consistent abundance diffusion treatment in the evolution of cooling white dwarfs permitted a study of the effect of elemental segregation in nonadiabatic, nonradial stability computations. In particular, mode trapping manifesting itself in cyclically varying period separations behaved differently from its appearance in the damping/excitation rates. Another aspect of the investigation concerned the effect of heavy-element traces in homogeneous DB white-dwarf envelopes on their pulsational instability domain. The stellar models are computed with the CGM convection approach; the study can therefore be considered as a test of its performance in nonradial stability analyses.

引用

页码：141 / 151

页数：11

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