NGC 507
NGC 507 | |
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![]() This image shows a vast cloud of hot gas (X-ray/red), surrounding high-energy bubbles (radio/blue) on either side of the bright white area around the supermassive black hole at the center of the galaxy. | |
Observation data | |
Constellation | Pisces |
Right ascension | 01h 23.7m 00s[1] |
Declination | +33° 15′ 00″[1] |
Redshift | 0.0165[2] |
Helio radial velocity | 4934 +/- 7 km/s[3] |
Galactocentric velocity | 5079 +/- 9 km/s[3] |
Distance | 227 million light years away[2] |
Apparent magnitude (V) | 11.3[1] |
Apparent magnitude (B) | 12.3[1] |
Surface brightness (specify) | 13.5[2] |
Characteristics | |
Type | E-S0[2] |
Apparent size (V) | 2.5 feet x 2.5 feet[2] |
Other designations | |
rp 229, CGCG 502-67, MCG 5-4-44, PGC 5098, UGC 938, V V 207 | |
NGC 507, also known as rp 229, CGCG 502-67, MCG 5-4-44, PGC 5098, UGC 938, and V V 207,[2] is a lenticular galaxy in the constellation Pisces. It was described as being "very faint", "pretty large", "round", "brighter in the middle", and "south of NGC 508" by John Dreyer in the New General Catalogue.[1] It was discovered by William Herschel on September 12, 1784.[4]
See also
External links
- NGC 507 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS
References
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