NGC 1369

Galaxy of the Fornax Cluster From Wikipedia, the free encyclopedia

NGC 1369 is a barred lenticular galaxy located 59 million light years away[4] in constellation of Eridanus. The galaxy was discovered by astronomer Julius Schmidt on January 19, 1865,[5] and is a member of the Fornax Cluster.[6] NGC 1369 is a host to a supermassive black hole with an estimated mass of 1.8 million solar masses.[7]

Quick facts Observation data (J2000 epoch), Constellation ...
NGC 1369
legacy surveys image of NGC 1369.
Observation data (J2000 epoch)
ConstellationEridanus (constellation)
Right ascension03h 36m 45.2s[1]
Declination−36° 15 22[1]
Redshift0.004717[1]
Heliocentric radial velocity1414 km/s[1]
Distance59 Mly (18.1 Mpc)[1]
Group or clusterFornax Cluster
Apparent magnitude (V)13.74[1]
Characteristics
TypeSB0/a(rs)[1]
Mass0.68×1010 (Stellar mass) [2]/3.5×1010 (Total Mass)[3] M
Size~25,800 ly (7.91 kpc) (estimated)[1]
Apparent size (V)1.5 x 1.4[1]
Other designations
ESO 358- G 034, MCG -06-09-004, FCC 176, PGC 013330[1]
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Surrounding NGC 1369 is a population of a least 11 known globular clusters.[8]

Physical characteristics

In the disk of NGC 1369, there are two bright, diffuse spiral arms which break of a relatively weak bar structure. These arms quickly fade in the diffuse outer disk.[9] Despite the presence of spiral arms, the galaxy is very red which actually makes NGC 1369 a lenticular galaxy.[10] Also, the galaxy is devoid of atomic and molecular gas,[11] and does not show any indications of ionised-gas emission as a result of star formation. Observations in X-rays have shown that it is infalling in a transional region of the Fornax Cluster between the high and low-density regions of the cluster where the X-ray emission is still present. As a result, ram-pressure stripping would have acted to stop star formation once the galaxy entered into the cluster core,[12] causing it to transion from a spiral galaxy to a lenticular galaxy.[11]

See also

References

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