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

被引：38

作者：

Barnes, SA ^{[1
]}

机构：

[1] Yale Univ, Dept Astron, New Haven, CT 06520 USA

来源：

ASTROPHYSICAL JOURNAL | 2003年 / 586卷 / 02期

基金：

美国国家科学基金会;

关键词：

open clusters and associations : general; stars : activity; stars : chromospheres; stars : late-type; stars : magnetic fields; stars : rotation;

D O I：

10.1086/374681

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

收藏

页码：L145 / L147

页数：3

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