NGC 4092是一个位于后发座的螺旋星系,距离地球3.1亿光年[2][3],1864年5月2日由海因里希·路易·达雷发现[4],属于NGC 4065星系群[5][6][7],有一个活动星系核[8]。
- ^ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 NASA/IPAC Extragalactic Database. Results for NGC 4092. [2019-02-12]. (原始内容存档于2008-12-16).
- ^ Your NED Search Results. ned.ipac.caltech.edu. [2019-02-13]. (原始内容存档于2022-06-30).
- ^ Revised NGC Data for NGC 4092. spider.seds.org. [2019-02-13]. (原始内容存档于2021-06-25).
- ^ New General Catalog Objects: NGC 4050 - 4099. cseligman.com. [2019-02-03]. (原始内容存档于2022-06-30).
- ^ Gregory, S. A.; Thompson, L. A. The Coma/A1367 supercluster and its environs. The Astrophysical Journal. 1978-06-01, 222: 784–799 [2022-06-30]. Bibcode:1978ApJ...222..784G. ISSN 0004-637X. doi:10.1086/156198. (原始内容存档于2017-09-23).
- ^ Tifft, W. G.; Gregory, S. A. Band theory applied to the Coma/A1367 supercluster. The Astrophysical Journal. 1979-07-01, 231: 23–27. Bibcode:1979ApJ...231...23T. ISSN 0004-637X. doi:10.1086/157158.
- ^ Burns, Jack O.; Hanisch, Robert J.; White, Richard A.; Nelson, Eric R.; Morrisette, Kim A.; Moody, J. Ward. A VLA 20 CM survey of poor groups of galaxies. The Astronomical Journal. 1987-09-01, 94: 587–617. Bibcode:1987AJ.....94..587B. ISSN 0004-6256. doi:10.1086/114494.
- ^ NGC 4092. sim-basic. [2019-02-13]. (原始内容存档于2022-06-30).