New nonadiabatic pulsation computations on full PG 1159 evolutionary models: the theoretical GW Virginis instability strip revisited
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20065423/pdf
Reference42 articles.
1. Low-temperature Rosseland opacities
2. The formation and evolution of hydrogen-deficient post-AGB white dwarfs: The emerging chemical profile and the expectations for the PG 1159-DB-DQ evolutionary connection
3. The pulsating nucleus of the planetary nebula Longmore 4
4. A Theoretical Analysis of Pulsation Driving in PG 1159 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
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3. Pulsating hydrogen-deficient white dwarfs and pre-white dwarfs observed with TESS;Astronomy & Astrophysics;2022-12
4. Kepler and TESS Observations of PG 1159-035;The Astrophysical Journal;2022-09-01
5. An evolutionary channel for CO-rich and pulsating He-rich subdwarfs;Monthly Notices of the Royal Astronomical Society: Letters;2022-01-07
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