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The planet-hosting subdwarf B star V 391 Pegasi is a hybrid pulsator

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Stahn,  T.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;

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Lutz, R., Schuh, S., Silvotti, R., Bernabei, S., Dreizler, S., Stahn, T., et al. (2009). The planet-hosting subdwarf B star V 391 Pegasi is a hybrid pulsator. Astronomy and Astrophysics, 496(2), 469-473. doi:10.1051/0004-6361/20079257.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0015-0246-3
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