NGC 6153
| 星云 | |
|---|---|
 | |
| 观测资料: J2000 epoch | |
| 分类 | II[3] |
| 赤经 | 16h 31m 30.57s[2] |
| 赤纬 | −40° 15′ 12.6″[2] |
| 距离 | 4,890 ± 980[4] 光年 |
| 视星等 (V) | 10.6[5] |
| 视直径 | 30″[5] |
| 星座 | 天蝎座 |
NGC 6153是位于南天星座天蝎座的一个行星状星云。英国天文学家罗夫·科普兰在1883年发现了它[6]。这个星云用孔径小到 80 mm（3.1英寸）就能看见，但丰富的银河系背景可能会使其难以找到。它的视星等为10.6，角直径跨度为30″[5]。
这是一个大致对称的双极星云，膨胀速度为12.7 to 17.3 km/s[7]。它包括一些结、细丝，可能还有双层壳结构[8]。NGC 6153属于Peimbert I型，表明它富含氦和氮，其前身是一颗薄盘恒星[9]。1986年对恒星光谱的分析表明，这是一个不寻常的星云。星云中几乎所有的元素，尤其是氮、氖、硫和氩，都过量了。在某些情况下，其丰度高于其它任何星云[7]。有人提出，这种差异是由于星云中的冷、富含金属、缺氢的结构造成的[10]。
对“盖亚”数据的分析表明，中心恒星可能是一个联星系统[11]。联星系统可以解释丰度差异[12]。在冷却轨迹上，白矮星可能会经历最后的热脉冲，导致恒星膨胀成一颗燃烧氦气的巨星，其演化轨迹与早期恒星几乎相同[13]。
参考文献
[编辑]- ^ A nitrogen-rich nebula. EAS/Hubble. [14 January 2025]. （原始内容存档于2018-09-11）.
- ^ 2.0 2.1 Brown, A. G. A.; et al. Gaia Early Data Release 3: Summary of the contents and survey properties. Astronomy & Astrophysics. 2021, 649: A1. Bibcode:2021A&A...649A...1G. S2CID 227254300. arXiv:2012.01533
. doi:10.1051/0004-6361/202039657 . 已忽略未知参数|collaboration=(帮助) (勘误: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR. - ^ Results for NGC 6153. VizieR Catalogue Database. [2013-09-06]. （原始内容存档于2016-03-04）.
- ^ Stanghellini, Letizia; Haywood, Misha. The Galactic Structure and Chemical Evolution Traced by the Population of Planetary Nebulae. The Astrophysical Journal. May 2010, 714 (2): 1096–1107. Bibcode:2010ApJ...714.1096S. arXiv:1003.0759 . doi:10.1088/0004-637X/714/2/1096.
- ^ 5.0 5.1 5.2 Griffiths, Martin. Planetary Nebulae and How to Observe Them. Springer New York. 2012: 253. ISBN 9781461417828.
- ^ Seligman, Courtney. New General Catalogue objects: NGC 6150 - 6199. cseligman.com. [27 September 2019]. （原始内容存档于2018-10-13）.
- ^ 7.0 7.1 Pottasch, S. R.; et al. Abundances in the planetary nebula NGC 6153. Astronomy and Astrophysics. February 1986, 155: 397–401. Bibcode:1986A&A...155..397P.
- ^ Anandarao, B. G.; Banerjee, D. P. K. High resolution observations of the planetary nebulae NGC 6153 and IC 4593. Astronomy and Astrophysics. August 1988, 202: 215–218. Bibcode:1988A&A...202..215A.
- ^ Quireza, C.; et al. Bayesian posterior classification of planetary nebulae according to the Peimbert types. Astronomy and Astrophysics. November 2007, 475 (1): 217–231. Bibcode:2007A&A...475..217Q. arXiv:0709.0711 . doi:10.1051/0004-6361:20078087.
- ^ Yuan, H. -B.; et al. Three-dimensional chemically homogeneous and bi-abundance photoionization models of the 'super-metal-rich' planetary nebula NGC 6153. Monthly Notices of the Royal Astronomical Society. February 2011, 411 (2): 1035–1052. Bibcode:2011MNRAS.411.1035Y. arXiv:1009.6148 . doi:10.1111/j.1365-2966.2010.17732.x .
- ^ Chornay, N.; et al. Towards a more complete sample of binary central stars of planetary nebulae with Gaia. Astronomy & Astrophysics. 2021, 648: A95. Bibcode:2021A&A...648A..95C. S2CID 230770301. arXiv:2101.01800 . doi:10.1051/0004-6361/202140288.
- ^ McNabb, I. A.; et al. Very Large Telescope deep echelle spectroscopy of Galactic planetary nebulae NGC 6153, M 1-42 and Hf 2-2. Monthly Notices of the Royal Astronomical Society. September 2016, 461 (3): 2818–2846. Bibcode:2016MNRAS.461.2818M. arXiv:1606.02925 . doi:10.1093/mnras/stw1405 .
- ^ Iben, I., Jr.; et al. On the evolution of those nuclei of planetary nebulae that experience a final helium shell flash. Astrophysical Journal. January 1983, 264: 605–612. Bibcode:1983ApJ...264..605I. doi:10.1086/160631.
进阶读物
[编辑]- Gómez-Llanos, V.; et al. MUSE spectroscopy of the high abundance discrepancy planetary nebula NGC 6153. Astronomy & Astrophysics. September 2024, 689. id. A228. Bibcode:2024A&A...689A.228G. arXiv:2407.06385 . doi:10.1051/0004-6361/202450822.
- Richer, Michael G.; et al. NGC 6153: Reality is Complicated. The Astronomical Journal. December 2022, 164 (6). id. 243. Bibcode:2022AJ....164..243R. arXiv:2210.05085 . doi:10.3847/1538-3881/ac9732 .
- Liu, X. -W.; et al. NGC 6153: a super-metal-rich planetary nebula?. Monthly Notices of the Royal Astronomical Society. March 2000, 312 (3): 585–628. Bibcode:2000MNRAS.312..585L. doi:10.1046/j.1365-8711.2000.03167.x .
- Liu, X. -W. Chemical Abundances of Planetary Nebulae: A UV to Far-IR Case Study of NGC 6153. Astrophysics and Space Science. 1998, 255 (1/2): 499–505. Bibcode:1998Ap&SS.255..499L. doi:10.1023/A:1001515704001.
外部链接
[编辑]
维基共享资源上的相关多媒体资源：NGC 6153- NGC 6153. SIMBAD. 斯特拉斯堡天文资料中心. [2013-09-06].
