A connection between the morphology of the X-ray emission and rotation for solar-type stars in open clusters

Preprint

28 March 2003

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0303632

Abstract

It is suggested that the three-segmented morphology of the soft X-ray emission from cluster and field stars may be understood in terms of the recent classification of rotating stars into three kinds: those lying on the convective sequence, on the interface sequence, or in the gap between them.

Keywords

CONVECTIVE SEQUENCE
CLASSIFICATION
X RAY EMISSION
OPEN CLUSTERS
MORPHOLOGY
SOLAR TYPE
SEGMENTED
STARS

All Related Versions

Version 1, 2003-03-28, ArXiv
Published version: The Astrophysical Journal, 586 (2), L145.

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