The stability of massive main-sequence stars
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/262/1/85/18539348/mnras262-0085.pdf
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1. Turbulent properties of Helium convective shells of massive stars;Monthly Notices of the Royal Astronomical Society;2021-04-06
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. No Detection of Strange Mode Pulsations in Massive Prime Candidate;Research Notes of the AAS;2018-09-12
4. Instability, finite amplitude pulsation and mass-loss in models of massive OB-type stars;Monthly Notices of the Royal Astronomical Society;2017-07-18
5. Strange mode instability driven finite amplitude pulsations and mass-loss in models of massive zero-age main-sequence stars;Monthly Notices of the Royal Astronomical Society;2016-10-23
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