NGC 1373

Galaxy in the constellation Fornax From Wikipedia, the free encyclopedia

NGC 1373 is a dwarf elliptical galaxy[4] located 61 million light years away[5] in constellation of Fornax. The galaxy was discovered by astronomer John Herschel on November 29, 1837,[6] and is a member of the Fornax Cluster.[7] NGC 1373 is a host to a supermassive black hole with an estimated mass of 4.6 million solar masses.[8]

Quick facts Observation data (J2000 epoch), Constellation ...
NGC 1373
DSS image of NGC 1373.
Observation data (J2000 epoch)
ConstellationFornax (constellation)
Right ascension03h 34m 59.2s[1]
Declination−35° 10 16[1]
Redshift0.004450[1]
Heliocentric radial velocity1334 km/s[1]
Distance61.13 Mly (18.744 Mpc)[1]
Group or clusterFornax Cluster
Apparent magnitude (V)14.1[1]
Absolute magnitude (V)−18.77[2]
Characteristics
TypeE+[1]
Mass1.3×109 (Stellar mass)/6×1010 (Total Mass)[3] M
Size~18,800 ly (5.76 kpc) (estimated)[1]
Apparent size (V)1.1 x 0.9[1]
Other designations
ESO 358- G 021, MCG -06-08-028, FCC 143, PGC 013252[1]
Close

63 known globular clusters have been observed surrounding NGC 1373,[9] along with 13 observed planetary nebulae.[10]

Physical characteristics

NGC 1373 is one of the most compact and faint elliptical galaxies in the Fornax Cluster.[11] As NGC 1373 is a compact elliptical galaxy, in the Fornax Cluster, it is expected to have older and more metal-rich populations of stars than similar compact elliptical galaxies of lower masses. It is thought that NGC 1373 originated as a more extended galaxy that transformed into a compact dwarf as it fell falling through the cluster.[12]

NGC 1373 appears to be interacting with the galaxy NGC 1374 and is separated from the galaxy by a distance of around 980,000 ly (0.3 Mpc).[10] This is evident as observations using the VLT Survey Telescope reveal the presence of a faint filament of matter connecting the two galaxies.[13]

See also

References

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