NGC 2232
| NGC 2232 | |
|---|---|
 NGC 2232 （摘自恒星库） | |
| 观测资料 (J2000 历元) | |
| 星座 | 麒麟座 |
| 赤经 | 06h 27m 15s[1] |
| 赤纬 | –04° 45′ 30″[1] |
| 距离 | 1,060 ly（325 pc）[2] |
| 视星等 (V) | 3.9[3] |
| 视大小 (V) | 30′ [3] |
| 物理特征 | |
| 质量 | < 100[4] M☉ |
| 半径 | ~15 ly[4] |
| 估计年龄 | 30.9 Myr[2] |
| 其他特征 | Cr 93, C 0624-047[5] |
NGC 2232是一个位于天球赤道附近的麒麟座，以麒麟-10为中心的一个明亮的疏散星团。[3] 它在猎户座大星云附近的古尔德带，[6]距太阳约1060光年。[2]该星系的平均径向速度为26.6±0.77 km/s。[7] NGC 2232 是距离太阳最近的疏散星团之一，是一个研究年轻恒星向主序星过渡的一个潜在目标之一。[8]
星团的角半径为36′，核心角半径为7.2′。是一个由20个集中恒星组成的稀疏簇[2] 。它被认为是一个超级太阳星团，该星团的恒星的铁含量通常比太阳更高，金属量为0.22±0.09或0.32±0.08，取决于所做的假设。[7] 至少四个恒星红外过量波长为8μm，为暖尘埃，其中HD 45435的波长超过24μm.，可能说明恒星处于早期演变阶段。[6]该星团中只有一颗恒星是特殊恒星。[9]
参考
- ^ 1.0 1.1 Wu, Zhen-Yu; et al, The orbits of open clusters in the Galaxy, Monthly Notices of the Royal Astronomical Society, November 2009, 399 (4): 2146–2164, Bibcode:2009MNRAS.399.2146W, S2CID 6066790, arXiv:0909.3737
, doi:10.1111/j.1365-2966.2009.15416.x.
- ^ 2.0 2.1 2.2 2.3 Kharchenko, N. V.; et al, Astrophysical parameters of Galactic open clusters, Astronomy and Astrophysics, 2005, 438 (3): 1163–1173, Bibcode:2005A&A...438.1163K, S2CID 9079873, arXiv:astro-ph/0501674 , doi:10.1051/0004-6361:20042523.
- ^ 3.0 3.1 3.2 Dunlop, Storm. Atlas of the Night Sky. Collins. 2005. ISBN 978-0-00-717223-8.
- ^ 4.0 4.1 Finlay, Warren H., Concise Catalog of Deep-sky Objects, The Patrick Moore Practical Astronomy Series 2nd, Springer Science & Business Media: 188, 2014, ISBN 978-3-319-03169-9.
- ^ NGC 2232. SIMBAD. 斯特拉斯堡天文资料中心. [2020-04-12].
- ^ 6.0 6.1 Currie, Thayne; et al, A Spitzer Study of Debris Disks in the Young Nearby Cluster NGC 2232: Icy Planets Are Common around ~1.5-3 M☉ Stars, The Astrophysical Journal, November 2008, 688 (1): 597–615, Bibcode:2008ApJ...688..597C, S2CID 28733060, arXiv:0807.2056 , doi:10.1086/591842.
- ^ 7.0 7.1 Monroe, TalaWanda R.; Pilachowski, Catherine A., Metallicities of Young Open Clusters. I. NGC 7160 and NGC 2232, The Astronomical Journal, December 2010, 140 (6): 2109–2123, Bibcode:2010AJ....140.2109M, S2CID 119241382, arXiv:1010.0739 , doi:10.1088/0004-6256/140/6/2109.
- ^ Orban, Chris; Patten, Brian, Late-Type Membership of the Open Cluster NGC 2232, Greenbelt, MD, United States: NASA Goddard Space Flight Center, January 1, 2004 [2020-04-13].
- ^ Jenkner, H.; Maitzen, H. M., Photoelectric search for CP2-stars in open clusters. X. NGC 2232, NGC2343, CR 140, and TR 10., Astronomy and Astrophysics, Supplemental Series, November 1987, 71: 255–261, Bibcode:1987A&AS...71..255J.
外部链接
维基共享资源上的相关多媒体资源：NGC 2232- Pang, Xiaoying; Li, Yuqian; Tang, Shih-Yun; Pasquato, Mario; Kouwenhoven, M. B. N. Different Fates of Young Star Clusters after Gas Expulsion. The Astrophysical Journal. 2020, 900 (1): L4. Bibcode:2020ApJ...900L...4P. S2CID 221083377. arXiv:2008.02803 . doi:10.3847/2041-8213/abad28.
