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

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.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0001-ADB5-0 Version Permalink: https://hdl.handle.net/21.11116/0000-0001-ADB6-F
Genre: Journal Article

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 Creators:
Lutz, R., Author
Schuh, S., Author
Silvotti, R., Author
Bernabei, S., Author
Dreizler, S., Author
Stahn, Thorsten1, Author           
Hügelmeyer, S. D., Author
Affiliations:
1Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832287              

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Language(s): eng - English
 Dates: 2009
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1051/0004-6361/20079257
 Degree: -

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Title: Astronomy and Astrophysics
  Other : Astron. Astrophys.
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: Berlin : Springer-Verlag
Pages: - Volume / Issue: 496 (2) Sequence Number: - Start / End Page: 469 - 473 Identifier: ISSN: 0004-6361
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219_1