A Driving Mechanism for the Newly Discovered Long‐Period Pulsating Subdwarf B Stars-Reference-Cited by-同舟云学术

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A Driving Mechanism for the Newly Discovered Long‐Period Pulsating Subdwarf B Stars

Published:2003-11 Issue:1 Volume:597 Page:518-534
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Fontaine G.,Brassard P.,Charpinet S.,Green E. M.,Chayer P.,Billeres M.,Randall S. K.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/597/i=1/a=518/pdf

Reference48 articles.

1. Detection ofp‐Mode Pulsations and Possible Ellipsoidal Luminosity Variations in the Hot Subdwarf B Star KPD 1930+2752

2. A Survey for Pulsating Hot B Subdwarfs in the Northern Hemisphere

3. Discovery and Asteroseismological Analysis of the Pulsating sdB Star PG 0014+067

4. The modeling of energy distributions and light curves of ZZ Ceti stars. 1: Basic theory and semianalytic expressions for the emergent flux

5. Adiabatic properties of pulsating DA white dwarfs. III - A finite-element code for solving nonradial pulsation equations

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