Time-resolved high-resolution spectroscopy of the pulsating sdB star QQ Vir (PG1325+101)

被引：0
|
作者：
J. Telting
R. Østensen
R. Oreiro
U. Heber
M. Vučković
S. Randall
A. Baran
机构：
[1] Nordic Optical Telescope,Instituut voor Sterrenkunde
[2] Katholieke Universiteit Leuven,Dr. Remeis Sternwarte Bamberg
[3] Universität Erlangen-Nürnberg,undefined
[4] European Southern Observatory,undefined
[5] Cracow Pedagogical University,undefined
来源：
Astrophysics and Space Science | 2010年 / 329卷
关键词：
Stellar pulsations; Subdarf B stars; QQ Vir (PG1325+101); Pulsation-mode identification; Time-resolved spectroscopy; Internal stellar structure; Stellar evolution;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
In March 2008 we obtained 2 nights of time-resolved high-resolution spectroscopy with UVES@VLT of the pulsating sdB QQ Vir (PG1325+101), totalling more than 750 spectra. We aim to study in detail the atmospheric response to the pulsations, and to derive observational constraints on the eigenmode of the main pulsation. In this paper we present the first preliminary results.
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页码：163 / 166
页数：3
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