The numerical simulation of non-linear non-radial stellar pulsations: a conservative formulation of gravity-Reference-Cited by-同舟云学术

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The numerical simulation of non-linear non-radial stellar pulsations: a conservative formulation of gravity

Published:2016-02-01 Issue:2 Volume:457 Page:1190-1197
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Glatzel W.,Chernigovski S.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/457/2/1190/2894360/stw003.pdf

Reference21 articles.

1. Chernigovski S. PhD thesis. Moscow State University; 1985.

2. A grid reconstruction procedure for the simulation of instabilities in luminous blue variables

3. The Piecewise Parabolic Method (PPM) for gas-dynamical simulations

4. Cox J. P. Theory of stellar pulsation. Princeton Univ. Press; Princeton, NJ; 1980.

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2. Instabilities and pulsations in models of the B-type supergiant κ Cassiopeiae (HD 2905);Monthly Notices of the Royal Astronomical Society;2020-11-21

3. Instability, finite amplitude pulsation and mass-loss in models of massive OB-type stars;Monthly Notices of the Royal Astronomical Society;2017-07-18

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