Surface activity of a Rossby sequence of cool Hyades stars

Fuente: arXiv
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Autori principali: Strassmeier, K. G., Ilyin, I., Steffen, M., Barnes, S. A.
Natura: Preprint
Pubblicazione: 2025
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author Strassmeier, K. G.
Ilyin, I.
Steffen, M.
Barnes, S. A.
author_facet Strassmeier, K. G.
Ilyin, I.
Steffen, M.
Barnes, S. A.
contents Aims. The Hyades cluster is key for the study of rotational, activity, and chemical evolution of solar-like low-mass stars. Here we present quantitative surface-activity information for a sequence of 21 Hyades dwarf stars. Conclusions. We conclude that the Rossby-number dependencies of the surface activity tracers A(Li), R(IRT), and B on our Hyades dwarf sequence primarily originate from convective motions, expressed by its turnover time, and only to a smaller and sometimes inverse extent from surface rotation and its related extra mixing.
format Preprint
id arxiv_https___arxiv_org_abs_2510_21456
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Surface activity of a Rossby sequence of cool Hyades stars
Strassmeier, K. G.
Ilyin, I.
Steffen, M.
Barnes, S. A.
Solar and Stellar Astrophysics
Aims. The Hyades cluster is key for the study of rotational, activity, and chemical evolution of solar-like low-mass stars. Here we present quantitative surface-activity information for a sequence of 21 Hyades dwarf stars. Conclusions. We conclude that the Rossby-number dependencies of the surface activity tracers A(Li), R(IRT), and B on our Hyades dwarf sequence primarily originate from convective motions, expressed by its turnover time, and only to a smaller and sometimes inverse extent from surface rotation and its related extra mixing.
title Surface activity of a Rossby sequence of cool Hyades stars
topic Solar and Stellar Astrophysics
url https://arxiv.org/abs/2510.21456