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The planet-hosting subdwarf B star V 391 Pegasi is a hybrid pulsator
Authors: Lutz, R.; Schuh, S.; Silvotti, R.; Bernabei, S.; Dreizler, S.; Stahn, T.; Huegelmeyer, S. D.
Date of Publication (YYYY-MM-DD): 2009
Title of Journal: Astronomy and Astrophysics
Volume: 496
Issue / Number: 2
Start Page: 469
End Page: 473
Document Type: Article
ID: 459669.0
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