A connection between the morphology of the x-ray emission and rotation for solar - type stars in open clusters
Mar, 20037 pages
Published in:
- Astrophys.J.Lett. 586 (2003) L145
e-Print:
- astro-ph/0303632 [astro-ph]
DOI:
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Abstract: (arXiv)
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.References(10)
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