NGC 1271

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NGC 1271
250px
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]
Helio radial velocity 5751 km/s[1]
Distance 249 Mly (76.3 Mpc)[1]
Group or cluster Perseus Cluster
Type E/SO[2]
Mass/Light ratio 1.35[3] M/L
Size (ly) ~14,000 ly (4.4 kpc) (estimated)[3]
Apparent dimensions (V) 0.567 x 0.306[1]
Apparent magnitude (V) 15.1[1]
Other designations
CGCG 540-96, PGC 12367[1]
See also: Galaxy, List of galaxies

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]

Supermassive Black Hole

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]

See also

External links

References

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