A seismic and gravitationally bound double star observed by Kepler. Implication 
for the presence of a convective core

Appourchaux, T.; Antia, H. M.; Ball, W.; Creevey, O.; Lebreton, Y.; Verma, K.; Vorontsov, S.; Campante, T. L.; Davies, G. R.; Gaulme, P.; Régulo, C.; Horch, E.; Howell, S.; Everett, M.; Ciardi, D.; Fossati, L.; Miglio, A.; Montalbán, J.; Chaplin, W. J.; García, R. A.; Gizon, L.

doi:10.1051/0004-6361/201526610

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A seismic and gravitationally bound double star observed by Kepler. Implication for the presence of a convective core

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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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Appourchaux, T., Antia, H. M., Ball, W., Creevey, O., Lebreton, Y., Verma, K., et al. (2015). A seismic and gravitationally bound double star observed by Kepler. Implication for the presence of a convective core. Astronomy and Astrophysics, 582: A25. doi:10.1051/0004-6361/201526610.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0029-33E7-F

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