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Cited article:

Periodic mass-loss episodes due to an oscillation mode with variable amplitude in the hot supergiant HD 50064

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Asteroseismology of OB stars with CoRoT

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Astronomische Nachrichten 331 (9-10) 1065 (2010)
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Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars

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Ground-based observations of the β Cephei CoRoT main target HD 180 642: abundance analysis and mode identification

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Astronomy & Astrophysics 506 (1) 269 (2009)
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CoRoT's view of newly discovered B-star pulsators: results for 358 candidate B pulsators from the initial run's exoplanet field data

P. Degroote, C. Aerts, M. Ollivier, et al.
Astronomy & Astrophysics 506 (1) 471 (2009)
https://doi.org/10.1051/0004-6361/200911884