Investigating magnetic activity of F stars with the Kepler mission

Bibcode
2014IAUS..302..222M
DOI
10.1017/S1743921314002130
Mathur, S.; García, R. A.; Ballot, J.; Ceillier, T.; Salabert, D.; Metcalfe, T. S.; Régulo, C.; Jiménez, A.; Bloemen, S.
Referencia bibliográfica

Magnetic Fields throughout Stellar Evolution, Proceedings of the International Astronomical Union, IAU Symposium, Volume 302, pp. 222-223

Fecha de publicación:
8
2014
Número de autores
9
Número de autores del IAC
2
Número de citas
1
Número de citas referidas
1
Descripción
The dynamo process is believed to drive the magnetic activity of stars like the Sun that have an outer convection zone. Large spectroscopic surveys showed that there is a relation between the rotation periods and the cycle periods: the longer the rotation period is, the longer the magnetic activity cycle period will be. We present the analysis of F stars observed by Kepler for which individual p modes have been measure and with surface rotation periods shorter than 12 days. We defined magnetic indicators and proxies based on photometric observations to help characterise the activity levels of the stars. With the Kepler data, we investigate the existence of stars with cycles (regular or not), stars with a modulation that could be related to magnetic activity, and stars that seem to show a flat behaviour.
Proyectos relacionados
Helio and Asteroseismologia
Sismología Solar y Estelar y Búsqueda de Exoplanetas

Los objetivos genéricos de este Proyecto son: 1) el estudio de la estructura y dinámica del interior solar, 2) la extensión de dicho estudio al caso de otras estrellas, 3) la búsqueda y caracterización de planetas extrasolares por métodos fotométricos (principalmente mediante el método de tránsitos) y espectroscópico (variaciones en la velocidad

Savita
Mathur
En ejecución
Tipo
Sin árbitro
Actividad estelar
Estrellas F
Física estelar e interestelar (FEEI)

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