英仙座OB1
外观
英仙座OB1 | |
---|---|
观测数据 | |
星座 | 英仙座 |
赤经 | 02h 21m[1] |
赤纬 | +57° 36′[1] |
平均距离 | 5.9 kly(1.8 kpc)[2] |
Span | 1,000 × 750 light years[3] |
径向速度 | −43.4[2] km/s |
物理性质 | |
成员 | 149[4] |
OB星 | ≥65[5] |
其它名称 | Per OB1[6] |
英仙座OB1是在北天球英仙座的一个OB星协。它以双星团(NGC 869和NGC 884)为中心[4],名称来源于银河系的英仙臂[7]。星协成员中最明亮的恒星是蓝超巨星大陵一(英仙座9)[3]。
参考资料
[编辑]- ^ 1.0 1.1 Sitnik, T. G. The Line-of-Sight Velocities of OB Associations and Molecular Clouds in a Wide Solar Neighborhood: The Streaming Motions of Stars and Gas in the Perseus Arm. Astronomy Letters. May 2003, 29: 311–320. Bibcode:2003AstL...29..311S. doi:10.1134/1.1573280.
- ^ 2.0 2.1 Mel'Nik, A. M.; Dambis, A. K. Kinematics of OB-associations and the new reduction of the Hipparcos data. Monthly Notices of the Royal Astronomical Society. 2009, 400 (1): 518. Bibcode:2009MNRAS.400..518M. arXiv:0909.0618 . doi:10.1111/j.1365-2966.2009.15484.x .
- ^ 3.0 3.1 Crossen, Craig; Rhemann, Gerald. Sky Vistas: Astronomy for Binoculars and Richest-Field Telescopes. Springer Science & Business Media. 2012: 93. ISBN 9783709106266.
- ^ 4.0 4.1 Lee, Hsu-Tai; Lim, Jeremy. On the Formation of Perseus OB1 at High Galactic Latitudes. The Astrophysical Journal. June 2008, 679 (2): 1352–1363. Bibcode:2008ApJ...679.1352L. arXiv:0804.4520 . doi:10.1086/587801.
- ^ Beech, Martin; Slawson, Robert W. Are There Really Blue Stragglers in Per OB1?. Astrophysics and Space Science. December 1995, 234 (2): 217–221. Bibcode:1995Ap&SS.234..217B. doi:10.1007/BF00627667.
- ^ Per OB1. SIMBAD. 斯特拉斯堡天文资料中心.
- ^ Inglis, Michael. Observer’s Guide to Star Clusters. New York, New York: Springer Science & Business Media. 2013: 184. ISBN 978-1-4614-7567-5.
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