CGCG 522-39, MCG 6-5-31, PGC 6962, UGC 1348, B2 0149+35[1]
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NGC 708 is an elliptical galaxy located 240 million light-years away[2] in the constellation Andromeda and was discovered by astronomer William Herschel on September 21, 1786.[3] It is classified as a cD galaxy[4][5] and is the brightest member of Abell 262.[6][7] NGC 708 is a weak[8] FR I radio galaxy[9][10][11][12][13] and is also classified as a type 2 Seyfert galaxy.[8][14][2]
NGC 708 is surrounded by 4,700 globular clusters.[15]
^ abcdefghij"NASA/IPAC Extragalactic Database". Results for NGC 708. Retrieved 2018-12-22.
^ ab"Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-12-23.
^"New General Catalog Objects: NGC 700 – 749". cseligman.com. Retrieved 2018-11-21.
^Lyskova, N.; Churazov, E.; Moiseev, A.; Sil'chenko, O.; Zhuravleva, I. (2014-05-15). "Stellar kinematics of X-ray bright massive elliptical galaxies". Monthly Notices of the Royal Astronomical Society. 441 (3): 2013–2033. arXiv:1404.2729. Bibcode:2014MNRAS.441.2013L. doi:10.1093/mnras/stu717. ISSN 0035-8711.
^Goullaud, Charles F.; Jensen, Joseph B.; Blakeslee, John P.; Ma, Chung-Pei; Greene, Jenny E.; Thomas, Jens (2018-03-20). "The MASSIVE Survey. IX. Photometric Analysis of 35 High-mass Early-type Galaxies with HST WFC3/IR". The Astrophysical Journal. 856 (1): 11. arXiv:1801.08245. Bibcode:2018ApJ...856...11G. doi:10.3847/1538-4357/aab1f3. ISSN 1538-4357. S2CID 119458429.
^West, M. J. (1994-05-01). "Anisotropic Mergers at High Redshifts - the Formation of CD Galaxies and Powerful Radio Sources". Monthly Notices of the Royal Astronomical Society. 268: 79–102. Bibcode:1994MNRAS.268...79W. doi:10.1093/mnras/268.1.79. ISSN 0035-8711.
^ abCite error: The named reference :7 was invoked but never defined (see the help page).
^Parma, P.; Morganti, R.; Fanti, R.; Ruiter, De; R, H.; Chiaberge, M.; Celotti, A.; Capetti, A. (2001-12-06). "The HST survey of the B2 sample of radio-galaxies: optical nuclei and the FRI/BL Lac unified scheme". Astronomy & Astrophysics. 383: 104–111. arXiv:astro-ph/0112151. Bibcode:2002A&A...383..104C. doi:10.1051/0004-6361:20011714. S2CID 2457431.
^Hu, C.; Wang, J.-M. (2005-08-01). "Captures of Red Giant Stars by Black Holes in Elliptical Galaxies: Feedback to the Hot Gas". The Astrophysical Journal. 630 (2): L125–L128. arXiv:astro-ph/0508021. Bibcode:2005ApJ...630L.125W. doi:10.1086/491670. S2CID 119078675.
^Clarke, T. E.; McNamara, Brian R.; Sarazin, Craig L.; Blanton, Elizabeth L. (2004-05-21). "Chandra Observation of the Central Region of the Cooling Flow Cluster Abell 262: A Radio Source that is a Shadow of its Former Self?". The Astrophysical Journal. 612 (2): 817–824. arXiv:astro-ph/0405425. Bibcode:2004ApJ...612..817B. doi:10.1086/422677. S2CID 2628446.
^Kassim, N. E.; Douglass, E. M.; Gopal-Krishna; Anderson, L. D.; Sarazin, C. L.; Blanton, E. L.; Clarke, T. E. (2009-03-04). "Tracing Multiple Generations of AGN Feedback in the Core of Abell 262". The Astrophysical Journal. 697 (2): 1481–1492. arXiv:0903.0844. Bibcode:2009ApJ...697.1481C. doi:10.1088/0004-637X/697/2/1481. S2CID 14636695.
^Cite error: The named reference :8 was invoked but never defined (see the help page).
^Reddy, Naveen A.; Yun, Min S. (2004-01-10). "Radio and Far-Infrared Emission as Tracers of Star Formation and AGN in Nearby Cluster Galaxies". The Astrophysical Journal. 600 (2): 695–715. arXiv:astro-ph/0309649. Bibcode:2004ApJ...600..695R. doi:10.1086/379871. ISSN 0004-637X. S2CID 15068448.
^Harris, William E.; Harris, Gretchen L. H.; Alessi, Matthew (2013-07-09). "A Catalog of Globular Cluster Systems: What Determines the Size of a Galaxy's Globular Cluster Population?". The Astrophysical Journal. 772 (2): 82. arXiv:1306.2247. Bibcode:2013ApJ...772...82H. doi:10.1088/0004-637X/772/2/82. ISSN 0004-637X. S2CID 119113886.
NGC708 is an elliptical galaxy located 240 million light-years away in the constellation Andromeda and was discovered by astronomer William Herschel...
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of the anomalous Cepheid in the globular cluster NGC 5466". The Astrophysical Journal. 262: 700–708. Bibcode:1982ApJ...262..700Z. doi:10.1086/160462.[permanent...
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