On the Driving Mechanism and the Coexistence of Variable and Nonvariable Stars in the Domain of the Pulsating PG 1159 Stars
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/610/i=1/a=436/pdf
Reference39 articles.
1. A Theoretical Analysis of Pulsation Driving in PG 1159 Stars
2. Brassard, P. & Fontaine, G. 1994, in IAU Colloq. 147, The Equation of State in Astrophysics, ed. G. Chabrier & E. Schatzman (Cambridge: Cambridge Univ. Press), 560
3. Adiabatic properties of pulsating DA white dwarfs. III - A finite-element code for solving nonradial pulsation equations
4. A Theoretical Exploration of the Pulsational Stability of Subdwarf B Stars
5. A Driving Mechanism for the Newly Discovered Class of Pulsating Subdwarf B Stars
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1. The GW Vir Instability Strip in Light of New Observations of PG 1159 Stars: Discovery of Pulsations in the Central Star of A72 and Variability of RX J0122.9–7521;The Astrophysical Journal Supplement Series;2023-11-01
2. Kepler and TESS Observations of PG 1159-035;The Astrophysical Journal;2022-09-01
3. The Missing Link? Discovery of Pulsations in the Nitrogen-rich PG 1159 Star PG 1144+005;The Astrophysical Journal Letters;2021-08-25
4. Asteroseismology of the GW Virginis stars SDSS J0349−0059 and VV 47;Astronomy & Astrophysics;2016-04-12
5. References;Pulsating Stars;2015-08-21
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