NGC 1271 | |
---|---|
![]()
SDSS image of NGC 1271 | |
Observation data ( J2000 epoch) | |
Constellation | Perseus |
Right ascension | 03h 19m 11.3s [1] |
Declination | 41° 21′ 12″ [1] |
Redshift | 0.019183 [1] |
Heliocentric radial velocity | 5751 km/s [1] |
Distance | 249 Mly (76.3 Mpc) [1] |
Group or cluster | Perseus Cluster |
Apparent magnitude (V) | 15.1 [1] |
Characteristics | |
Type | E/SO [2] |
Mass/Light ratio | 1.35 [3] M☉/ L☉ |
Size | ~14,000 ly (4.4 kpc) (estimated) [3] |
Apparent size (V) | 0.567 x 0.306 [1] |
Other designations | |
CGCG 540-96, PGC 12367 [1] |
NGC 1271 is a compact elliptical or lenticular galaxy [2] located about 250 million light-years away [4] in the constellation Perseus. [5] The galaxy was discovered by astronomer Guillaume Bigourdan on November 14, 1884. [6] NGC 1271 is a member of the Perseus Cluster [7] [6] and has a nuclear dust disk in its center. [3] It also has an edge-on, intermediate-scale disk and has a central bulge. [2] Like NGC 1277, NGC 1271 is a candidate " relic galaxy". [8]
Using orbital-based stellar dynamical models, Walsh et al. determined that the
supermassive black hole in the center of NGC 1271 has a mass of 3.0+1.0
−1.1×109
M☉.
[3]
NGC 1271 | |
---|---|
![]()
SDSS image of NGC 1271 | |
Observation data ( J2000 epoch) | |
Constellation | Perseus |
Right ascension | 03h 19m 11.3s [1] |
Declination | 41° 21′ 12″ [1] |
Redshift | 0.019183 [1] |
Heliocentric radial velocity | 5751 km/s [1] |
Distance | 249 Mly (76.3 Mpc) [1] |
Group or cluster | Perseus Cluster |
Apparent magnitude (V) | 15.1 [1] |
Characteristics | |
Type | E/SO [2] |
Mass/Light ratio | 1.35 [3] M☉/ L☉ |
Size | ~14,000 ly (4.4 kpc) (estimated) [3] |
Apparent size (V) | 0.567 x 0.306 [1] |
Other designations | |
CGCG 540-96, PGC 12367 [1] |
NGC 1271 is a compact elliptical or lenticular galaxy [2] located about 250 million light-years away [4] in the constellation Perseus. [5] The galaxy was discovered by astronomer Guillaume Bigourdan on November 14, 1884. [6] NGC 1271 is a member of the Perseus Cluster [7] [6] and has a nuclear dust disk in its center. [3] It also has an edge-on, intermediate-scale disk and has a central bulge. [2] Like NGC 1277, NGC 1271 is a candidate " relic galaxy". [8]
Using orbital-based stellar dynamical models, Walsh et al. determined that the
supermassive black hole in the center of NGC 1271 has a mass of 3.0+1.0
−1.1×109
M☉.
[3]