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  Rotation periods of 12 000 main-sequence Kepler stars: Dependence on stellar spectral type and comparison with v sin i observations

Nielsen, M. B., Gizon, L., Schunker, H., & Karoff, C. (2013). Rotation periods of 12 000 main-sequence Kepler stars: Dependence on stellar spectral type and comparison with v sin i observations. Astronomy and Astrophysics, 557: L10. doi:10.1051/0004-6361/201321912.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0015-0B91-B Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0015-0B92-9
Genre: Journal Article

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 Creators:
Nielsen, M. B.1, Author              
Gizon, L.1, Author              
Schunker, H.1, Author              
Karoff, C., Author
Affiliations:
1Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832287              

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 MPIS_GROUPS: Solar and Stellar Interiors
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 Dates: 2013
 Publication Status: Published in print
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 Rev. Method: Peer
 Identifiers: DOI: 10.1051/0004-6361/201321912
BibTex Citekey: Nielsen:2013-092
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Title: Astronomy and Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 557 Sequence Number: L10 Start / End Page: - Identifier: -