TOWARD HIGH-PRECISION SEISMIC STUDIES OF WHITE DWARF STARS: PARAMETRIZATION OF THE CORE AND TESTS OF ACCURACY
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/834/i=2/a=136/pdf
Reference35 articles.
1. A New Method of Interpolation and Smooth Curve Fitting Based on Local Procedures
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3. Evolution of a 3-M⊙star from the main sequence to the ZZ Ceti stage: the role played by element diffusion
4. KIC 4552982: OUTBURSTS AND ASTEROSEISMOLOGY FROM THE LONGEST PSEUDO-CONTINUOUS LIGHT CURVE OF A ZZ Ceti
5. Theoretical Models for Asteroseismology of DA White Dwarf Stars
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1. Properties and asteroseismological analysis of a new ZZ ceti discovered by TMTS;Monthly Notices of the Royal Astronomical Society;2023-05-22
2. Asteroseismology of the Pulsating Extremely Low-mass White Dwarf SDSS J111215.82 + 111745.0: A Model with p-mode Pulsations Consistent with the Observations;The Astrophysical Journal;2023-01-31
3. New DA white dwarf models for asteroseismology of ZZ Ceti stars;Astronomy & Astrophysics;2022-07
4. Seismic Cartography of White-Dwarf Interiors From the Toulouse-Montréal Optimal-Design Approach;Frontiers in Astronomy and Space Sciences;2022-06-14
5. Asteroseismological Analysis of the DAV HS 0507+0434B: The Influence of Chemical Profile on the Pulsation Periods;The Astrophysical Journal;2021-11-26
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