NGC 4874

Coma A
NGC 4874 dominates this picture created from optical and near-infrared exposures taken with the Wide Field Channel of Hubble's Advanced Camera for Surveys.
Observation data (J2000 epoch)
Constellation	Coma Berenices
Right ascension	12^h 59^m 35.709^s^[1]
Declination	+27° 57′ 33.80″^[1]
Redshift	0.23937
Distance	109 Mpc (360 Mly)^[2]
Type	cD, Ei, E0
Apparent magnitude (V)	12.7
Other designations
NGC 4874, NFP J125935.7+275734, [BGH2001] 237, [KK90] 169, B2 1257+28, 10P 236, [BO85] Coma 1, [L84] A1656-G2, 5C 4.85, SDSS J125935.70+275733.3, [BTM97] ACO 1656 2, [LGF2005] B125711+281340, CAIRNS J125935.60+275734.0, TT 12, [CHM2007] LDC 926 J125935.70+2757338, [LO95] 1257+282, FOCA 0728-499, UGC 8103, [CHM2007] HDC 745 J125935.70+2757338, [MHR2010] 194.8988+27.9593, GIN 765, UZC J125935.6+275734, [D80] ACO 1656 129, [MO2001b] J125935.7+275732.3, GMP 3329, 4W 1257+28W01, [DFO95] 246, [MOL2003] A1656 J125935+275730, GP 489, 7W 1257+28W01, [DLB87] C11, [OLK95] 1257+282, LEDA 44628, WSTB 74W16, [EDG2007] 3, [OR76] 1257+282, 2MASX J12593562+2757360, Z 1257.2+2814, [FBH2004] X281, [OSR2002] b089, 2MASX J12593570+2757338, Z 160-A22, [FBH2004] S89, [PL95] ACO 1656 G2, MCG+05-31-070, Z 160A-22, [FWB89] Galaxy 321, [ZBO89] ACO 1656-5, MPMM 123, Z 160-231, [K94] 125710.70+281346.0

NGC 4874 (Coma A) is a supergiant elliptical galaxy. It was discovered by the British astronomer Frederick William Herschel I in 1785, who catalogued it as a bright patch of nebulous feature. The second brightest galaxy within the northern Coma Cluster, it is located at a distance of 109 megaparsecs (350 million light years) from Earth. Unlike a disc-shaped spiral galaxy like the Milky Way, NGC 4874 has no extensive dust lanes or spiral arms and has a smooth, featureless, ball-shaped profile that diminishes in luminosity with distance from the center. The galaxy is surrounded by an immense stellar halo that extends up to 1 million light years in diameter. It is also enveloped by a huge cloud of interstellar medium that is currently being heated by action of infalling material from its central supermassive black hole. A jet of highly energetic plasma extends out to 1,700 light years from its center.

References

1 2 "SIMBAD basic query result". SIMBAD Astronomical Database. Retrieved 20 September 2011.
↑ "Galaxies in a Swarm of Star Clusters". Picture of the Week. ESA/Hubble. Retrieved 20 September 2011.

Astronomical catalogs

NGC	NGC 4869 NGC 4870 NGC 4871 NGC 4872 NGC 4873 NGC 4874 NGC 4875 NGC 4876 NGC 4877 NGC 4878 NGC 4879

New General Catalogue 4500 to 4999

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Astronomical catalog List of NGC objects

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