OBSERVATIONAL SIGNATURES OF CONVECTIVELY DRIVEN WAVES IN MASSIVE STARS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.1088/2041-8205/806/2/L33/pdf
Reference34 articles.
1. Massive Star Asteroseismology in Action
2. Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars
3. On the use of the Fourier transform to determine the projected rotational velocity of line-profile variable B stars
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