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

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

2003-03-28

arxiv.org/abs/astro-ph/0303632v1

Astrophys.J. 586 (2003) L145

Astronomy and Astrophysics

Astrophysics

7 pages, 1 (color) figure, accepted by ApJ Letters

Scientific paper

10.1086/374681

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.

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