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.

doi:10.1051/0004-6361/201321912

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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

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Nielsen, M. B.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;

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Gizon, L.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;

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Schunker, H.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;

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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.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-0B91-B

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