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Cited article:
S. Mathis , V. Prat
A&A, 631 (2019) A26
Published online: 2019-10-15
This article has been cited by the following article(s):
19 articles
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Probing the interior physics of stars through asteroseismology
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Rossby numbers and stiffness values inferred from gravity-mode asteroseismology of rotating F- and B-type dwarfs
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Detecting axisymmetric magnetic fields using gravity modes in intermediate-mass stars
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Transport of angular momentum by stochastically excited waves as an explanation for the outburst of the rapidly rotating Be star HD49330
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