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Stellar activity in open clusters

Published online by Cambridge University Press:  23 December 2024

A. Görgei Open the ORCID record for A. Görgei [Opens in a new window] ,
K. Vida Open the ORCID record for K. Vida [Opens in a new window] ,
B. Seli  and
L. Kriskovics
A. Görgei*
Affiliation:
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, Hungary CSFK, MTA Centre of Excellence, Budapest, Hungary Eötvös Loránd University, Budapest, Hungary
K. Vida
Affiliation:
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, Hungary CSFK, MTA Centre of Excellence, Budapest, Hungary
B. Seli
Affiliation:
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, Hungary CSFK, MTA Centre of Excellence, Budapest, Hungary Eötvös Loránd University, Budapest, Hungary
L. Kriskovics
Affiliation:
Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Budapest, Hungary CSFK, MTA Centre of Excellence, Budapest, Hungary
*
email: [email protected]
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Abstract

Stellar activity depends on multiple parameters one of which is the age of the star. The members of open clusters are good targets to observe the activity at a given age of the stars since their ages are more precisely determined than that of field stars. Choosing multiple clusters, each with different age, gives us insight to the change in activity during the lifetime of stars. With the analysis of these stars we can also refine the parameters of gyrochronology (Barnes 2003), which is a method for estimating the age of low-mass, main sequence stars from their rotation periods.

Keywords

Stars: activityrotationmethods: data analysistechniques: photometry
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 19 , Symposium S365: Dynamics of Solar and Stellar Convection Zones and Atmospheres , December 2023 , pp. 436 - 440
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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