NGC 1512

Galaxy in the constellation Horologium From Wikipedia, the free encyclopedia

NGC 1512 is a barred spiral galaxy approximately 38 million light-years away from Earth[2] in the constellation Horologium. It was discovered by Scottish astronomer James Dunlop on 29 October 1826.[3]

Right ascension04h 03m 54.1662s[1]
Declination−43° 20 55.658[1]
Redshift0.002995±0.0000100[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 1512
Observation data (J2000 epoch)
ConstellationHorologium
Right ascension04h 03m 54.1662s[1]
Declination−43° 20 55.658[1]
Redshift0.002995±0.0000100[1]
Heliocentric radial velocity898±3 km/s[1]
Distance11.6 Mpc (38 Mly) h1
0.73
[2]
Apparent magnitude (V)11.1[1]
Characteristics
TypeSB(r)ab[1]
Size213,140 ly (65.38 kpc) (estimated)[1]
Apparent size (V)8.9 × 5.6[1]
Other designations
ESO 250- G 004, IRAS 04022-4329, 2MASX J04035428-4320558, MCG -07-09-007, PGC 14391[1]
Close

The galaxy displays a double ring structure, with a (nuclear) ring around the galactic nucleus and an (inner) further out in the main disk. The galaxy hosts an extended UV disc with at least 200 clusters with recent star formation activity.[4] NGC 1512 is a member of the Dorado Group.[5]

Gravitational interaction with NGC 1510

Gravitational tidal forces of NGC 1512 are influencing nearby dwarf lenticular galaxy NGC 1510. The two galaxies are separated by only ~5 arcmin (13.8 kpc),[4] and are in the process of a lengthy merger which has been going on for 400 million years.[6] At the end of this process NGC 1512 will have cannibalised its smaller companion.[7]

Interaction between these two galaxies has triggered star formation activity in the outskirts of the disc and enhanced the tidal distortion in the arms of the NGC 1512. The interaction seems to occur in the north-western areas of the system because of the broadening of the H i arm and the spread of the UV-rich star clusters in this region.[4]

See also

References

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