UGC 4653

Trio of interacting galaxies in the constellation Lynx From Wikipedia, the free encyclopedia

UGC 4653 known as Arp 195, is a trio of interacting galaxies located 763 million light-years away from the Solar System in the Lynx constellation.[1] The galaxies are being distorted through gravitational interactions with each other.[2][3] The first known reference for this object, was in 1959 where B.A. Vorontsov-Vel'yaminov compiled it inside the Vorontsov-Vel'yaminov Interacting galaxies, as VV 243.[4]

Right ascension08h 53m 54.6s[1]
Declination+35° 09 00[1]
Redshift0.056836[1]
Quick facts Observation data (J2000 epoch), Constellation ...
UGC 4653
Hubble Space Telescope image of UGC 4653
Observation data (J2000 epoch)
ConstellationLynx
Right ascension08h 53m 54.6s[1]
Declination+35° 09 00[1]
Redshift0.056836[1]
Heliocentric radial velocity16,748 km/s[1]
Distance763 Mly (233.9 Mpc)
Apparent magnitude (V)0.093
Apparent magnitude (B)0.124
Characteristics
TypeSB(s)b[1]
Size~440,000 ly (135 kpc) (estimated)[1]
Apparent size (V)1.9' x 1.1'
Notable featuresInteracting galaxy
Other designations
PGC 24981, SDSS J085354.62+350844.0, 2MASX J08535462+3508439, Arp 195, LEDA 24981, MCG+06-20-012, VV 243[1]
Close

This image of UGC 4653 was captured by the Hubble Space Telescope.[2] The galaxies make up the 195th object in the Atlas of Peculiar Galaxies created by Halton Arp.[5] They fall into the category of galaxies with material ejected from nuclei.[6]

UGC 4653 has active nuclear regions which produce infrared (IR) emissions.[7] These appear to be more like AGNs than HII regions.[7]

A study published in 2023, confirmed all three galaxies of the UGC 4653 system are spirals. The southern galaxy is a face-on galaxy hosting a bright core, while the central is edge-on but no clear distinction whether it is an early or late-type galaxy. The northern galaxy has a tidal tail and is of late-type morphology. With the exception of the third, both galaxies contain presence of strong emission lines.[8]

Supernova

Type Ia supernova, SN 2008bv[9] was discovered in UGC 4653 with a magnitude of 18.3.[10] It was located 1".7 east and 3".9 south of the nucleus.[11]

References

Related Articles

Wikiwand AI