The stability of massive main-sequence stars as a function of metallicity
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/423/4/3397/4900927/mnras0423-3397.pdf
Reference31 articles.
1. Pulsational stability of stars in thermal imbalance. VI - Physical mechanisms and extension to nonradial oscillations
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3. Radiation-driven winds in Of stars
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