期刊
ASTROPHYSICAL JOURNAL
卷 586, 期 2, 页码 L145-L147出版社
UNIV CHICAGO PRESS
DOI: 10.1086/374681
关键词
open clusters and associations : general; stars : activity; stars : chromospheres; stars : late-type; stars : magnetic fields; stars : rotation
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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