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          Institute: MPI für Sonnensystemforschung     Collection: Helioseismology Studies     Display Documents



ID: 459669.0, MPI für Sonnensystemforschung / Helioseismology Studies
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.
Research Context:Project(s) = none, Nachwuchs, ref
Date of Publication (YYYY-MM-DD):2009
Title of Journal:Astronomy and Astrophysics
Volume:496
Issue / Number:2
Start Page:469
End Page:473
Review Status:Peer-review
Audience:Experts Only
Intended Educational Use:No
External Publication Status:published
Document Type:Article
Communicated by:Patrick Daly
Affiliations:MPI für Sonnensystemforschung/Helioseismology Studies
Identifiers:LOCALID:Lutz:2009-190
DOI:10.1051/0004-6361/20079257
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