Rotation and magnetism of Kepler pulsating solar-like stars: towards asteroseismically calibrated age-rotation relations

Kepler ultra-high precision photometry of long and continuous observations provides a unique dataset in which surface rotation and variability can be studied for thousands of stars. Because many of these old field stars also have independently measured asteroseismic ages, measurements of rotation an...

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Bibliografiska uppgifter
Huvudupphovsmän: García, R. A., Ceillier, T., Salabert, D., Mathur, S., van Saders, J. L., Pinsonneault, M., Ballot, J., Beck, P. G., Bloemen, S., Campante, T. L., G. R., Davies, Nascimento Júnior, José Dias do, S., Mathis, Metcalfe, T. S., M. B., Nielsen, J. C., Suárez, W. J., Chaplin, A., Jiménez
Materialtyp: article
Språk:English
Publicerad: EDP Sciences
Ämnen:
Asteroseismology
Stars - activity
stars - rotation
stars - solar-type
stars - evolution
stars - oscillations
Länkar:https://repositorio.ufrn.br/jspui/handle/123456789/29011
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https://repositorio.ufrn.br/jspui/handle/123456789/29011

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