NGC 2362
| NGC 2362 | |
|---|---|
 NGC 2362 Credit: NASA/JPL-Caltech/Harvard-Smithsonian CfA | |
| 观测数据 (J2000 历元) | |
| 星座 | 大犬座 |
| 赤经 | 07h 18.6m[1] |
| 赤纬 | –24° 59′[1] |
| 距离 | (4.8 ± 1.6)×103 光年 ((1.5 ± 0.5)×103秒差距[2]) |
| 物理性质 | |
| 相关条目：疏散星团、疏散星团列表 | |
NGC 2362是位于大犬座的疏散星团。它在1654年之前就已经被意大利天文学家乔瓦尼·巴蒂斯特·霍迪尔纳首先观测到。
在NGC 2362中，最亮的恒星是大犬座τ星，因此这个疏散星团有时候也被称为大犬座τ星团。这个星团距离地球约1480秒差距（4800光年），年龄大约为400万－500万年，质量大于500个太阳质量[3]。
参见
参考资料
- ^ 1.0 1.1 NGC 2362 -- Open (galactic) Cluster. SIMBAD. Centre de Données astronomiques de Strasbourg. [2010-03-07]. （原始内容存档于2016-03-12）.
- ^ Lada, Charles J.; Reid, Mark J. CO observations of a molecular cloud complex associated with the bright rim near VY Canis Majoris. The Astrophysical Journal (American Astronomical Society). January 1, 1978, 219: 95–104. Bibcode:1978ApJ...219...95L. doi:10.1086/155758.
- ^ Currie, Thayne; et al.. The Last Gasp of Gas Giant Planet Formation: A Spitzer Study of the 5 Myr Old Cluster NGC 2362. The Astrophysical Journal. June 2009, 698 (1): 1–27. Bibcode:2009ApJ...698....1C. doi:10.1088/0004-637X/698/1/1.
- ^ Lada, C. J.; Reid, M. J. CO observations of a molecular cloud complex associated with the bright rim near VY Canis Majoris. Astrophysical Journal. January 1978, 219: 95–97, 99–104. Bibcode:1978ApJ...219...95L. doi:10.1086/155758.
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