NGC 1271 是英仙座的一个椭圆星系或透镜状星系[1]。距地球约 2.5 亿光年[2]。该星系由天文学家纪尧姆·比古尔丹于 1884 年 11 月 14 日发现。[3] NGC 1271是英仙座星系团的一员[4][5]。其中心有一个核球。[6]
参考文献
- ^ Graham, Alister W.; Ciambur, Bogdan C.; Savorgnan, Giulia A. D. Disky Elliptical Galaxies and the Allegedly Over-massive Black Hole in the Compact "ES" Galaxy NGC 1271. The Astrophysical Journal. 2016, 831 (2): 132. Bibcode:2016ApJ...831..132G. ISSN 0004-637X. S2CID 118435675. arXiv:1608.00711
. doi:10.3847/0004-637X/831/2/132 （英语）.
- ^ Your NED Search Results. ned.ipac.caltech.edu. [2018-06-23]. （原始内容存档于2023-08-22）.
- ^ New General Catalog Objects: NGC 1250 - 1299. cseligman.com. [2018-06-15]. （原始内容存档于2010-06-28） （美国英语）.
- ^ Brunzendorf, J.; Meusinger, H. The galaxy cluster Abell 426 (Perseus). A catalogue of 660 galaxy positions, isophotal magnitudes and morphological types. Astronomy and Astrophysics Supplement Series. October 1, 1999, 139 (1): 141–161. Bibcode:1999A&AS..139..141B. ISSN 0365-0138. doi:10.1051/aas:1999111 （英语）.
- ^ Walsh, Jonelle L.; Bosch, Remco C. E. van den; Gebhardt, Karl; Yildirim, Akin; Gültekin, Kayhan; Husemann, Bernd; Richstone, Douglas O. The Black Hole in the Compact, High-Dispersion Galaxy NGC 1271. The Astrophysical Journal. 2015-08-03, 808 (2): 183. Bibcode:2015ApJ...808..183W. ISSN 1538-4357. S2CID 41570998. arXiv:1506.05129 . doi:10.1088/0004-637X/808/2/183 （英语）.
- ^ Ferré-Mateu, Anna; Mezcua, Mar; Trujillo, Ignacio; Balcells, Marc; Bosch, Remco C. E. van den. Massive Relic Galaxies Challenge the Co-evolution of Super-massive Black Holes and Their Host Galaxies. The Astrophysical Journal. 2015, 808 (1): 79. Bibcode:2015ApJ...808...79F. ISSN 0004-637X. S2CID 118777377. arXiv:1506.02663 . doi:10.1088/0004-637X/808/1/79 （英语）.
维基共享资源上的相关多媒体资源：NGC 1271
