Pulsational instability of high-luminosity H-rich pre-white dwarf star-Reference-Cited by-同舟云学术

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Pulsational instability of high-luminosity H-rich pre-white dwarf star

Published:2017 Issue: Volume:152 Page:06012
ISSN:2100-014X
Container-title:EPJ Web of Conferences
language:
Short-container-title:EPJ Web Conf.

Author:

Calcaferro Leila M.,Córsico Alejandro H.,Camisassa María E.,Althaus Leandro G.,Shibahashi Hiromoto

Publisher

EDP Sciences

Link

http://www.epj-conferences.org/10.1051/epjconf/201715206012/pdf

Reference7 articles.

1. White dwarf evolutionary sequences for low-metallicity progenitors: The impact of third dredge-up

2. Pulsations powered by hydrogen shell burning in white dwarfs

3. New nonadiabatic pulsation computations on full PG 1159 evolutionary models: the theoretical GW Virginis instability strip revisited

4. SPECTROSCOPIC ANALYSIS OF HOT, HYDROGEN-RICH WHITE DWARFS: THE PRESENCE OF METALS AND THE BALMER-LINE PROBLEM

5. The helium shell game - Nonradial g-mode instabilities in hydrogen-deficient planetary nebula nuclei

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A new instability domain of CNO-flashing low-mass He-core stars on their early white-dwarf cooling branches;Astronomy & Astrophysics;2021-03

2. White-Dwarf Asteroseismology With the Kepler Space Telescope;Frontiers in Astronomy and Space Sciences;2020-08-28

3. Pulsating white dwarfs: new insights;The Astronomy and Astrophysics Review;2019-09-03

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