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| Query : 2003ApJ...586L.145B |
2003ApJ...586L.145B - Astrophys. J., 586, L145-L147 (2003/April-1)
A connection between the morphology of the X-ray emission and rotation for solar-type stars in open clusters.
BARNES S.A.
Abstract (from CDS):
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.
Abstract Copyright: ∼
Journal keyword(s): Galaxy: Open Clusters and Associations: General - Stars: Activity - Stars: Chromospheres - Stars: Late-Type - Stars: Magnetic Fields - Stars: Rotation
Simbad objects: 3
| Number of rows : 3 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | Cl Melotte 20 | MGr | 03 26 50.6 | +48 51 48 | ~ | 928 | 0 | |||||
| 2 | IC 2391 | OpC | 08 41 17.5 | -53 03 00 | ~ | 871 | 0 | |||||
| 3 | IC 2602 | OpC | 10 42 55.9 | -64 25 22 | ~ | 735 | 0 |
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