Asteroseismology of the Crystallized ZZ Ceti Star BPM 37093: A Different View
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/622/i=1/a=572/pdf
Reference19 articles.
1. On the Purity of the ZZ Ceti Instability Strip: Discovery of More Pulsating DA White Dwarfs on the Basis of Optical Spectroscopy
2. Photometric and Spectroscopic Analysis of Cool White Dwarfs with Trigonometric Parallax Measurements
3. Optical and Ultraviolet Analyses of ZZ Ceti Stars and Study of the Atmospheric Convective Efficiency in DA White Dwarfs
4. 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
5. Discovery and Asteroseismological Analysis of the Pulsating sdB Star PG 0014+067
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2. Cubic crystal elastic constants of a white dwarf stellar core determined via modal analysis;AIP Advances;2021-10-01
3. Asteroseismological analysis of the ultra-massive ZZ Ceti stars BPM 37093, GD 518, and SDSS J0840+5222;Astronomy & Astrophysics;2019-12
4. Evolution and asteroseismology of ultra-massive DA white dwarfs;Proceedings of the International Astronomical Union;2019-10
5. Pulsating white dwarfs: new insights;The Astronomy and Astrophysics Review;2019-09-03
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