Asteroseismology of hybridδScuti-γDoradus pulsating stars
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201629126/pdf
Reference103 articles.
1. Aerts, C., Christensen-Dalsgaard, J., & Kurtz, D. W. 2010, Asteroseismology, Astron. Astrophys. Lib. (Springer)
2. New evolutionary models for massive ZZ Ceti stars. I. First results for their pulsational properties
3. 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
4. Evolutionary and pulsational properties of white dwarf stars
5. New phase diagrams for dense carbon-oxygen mixtures and white dwarf evolution
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1. Two High-amplitude δ Scuti–γ Doradus Hybrids Constrained by the Radial Fundamental p and Equally Spaced g Modes;The Astrophysical Journal;2024-03-01
2. A grid of 200 000 models of young δ Scuti stars using mesa and GYRE;Monthly Notices of the Royal Astronomical Society;2023-09-25
3. Frequency analysis of the hybrid δ Sct-γ Dor star CoRoT-102314644;Astronomy & Astrophysics;2023-08
4. Convective Boundary Mixing in Main-Sequence Stars: Theory and Empirical Constraints;Galaxies;2023-04-14
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