UGC 4653
| UGC 4653 | |
|---|---|
 Hubble image of UGC 4653 | |
| Observation data | |
| Constellation | Lynx |
| Right ascension | 133.47 degree |
| Declination | 35.14 degree |
| Redshift | 0.056836 0.00143 |
| Heliocentric radial velocity | 16,748 km/s |
| Distance | 763 Mly (233.9 Mpc) |
| Apparent magnitude (V) | 13.645 0.004 |
| Notable features | Interacting galaxy |
| Other designations | |
| PGC 24981, SDSS J085354.62+350844.0, 2MASX J08535462+3508439, Arp 195, LEDA 24981, MCG+06-20-012, VV 243 | |
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]
This image was captured by the Hubble Space Telescope.[2] The galaxies make up the 195th object in the Atlas of Peculiar Galaxies which was created by Halton Arp.[3] They fall into the category of galaxies with material ejected from nuclei.[4]
UGC 4653 has active nuclear regions which produce infrared (IR) emissions.[5] These appear to be more like AGNs than HII regions.[5]
Supernova[edit]
Type Ia supernova, SN 2008bv[6] was discovered in UGC 4653 with a magnitude of 18.3.[7] It was located 1".7 east and 3".9 south of the nucleus.[8]
References[edit]
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-21.
- ^ a b information@eso.org. "Squabbling Galactic Siblings". www.spacetelescope.org. Retrieved 2024-04-21.
- ^ "Halton Arp's Atlas of Peculiar Galaxies". cseligman.com. Retrieved 2024-04-21.
- ^ "Arp 195 - Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets, Telescopes". cs.astronomy.com. Retrieved 2024-04-21.
- ^ a b Fiorenza, Stephanie; Uzan, Raphael. "A Study of the Nuclear Regions of the Triple Merging System Arp 195". Astrophysics Data System. Retrieved 27 April 2024.
- ^ Li, W.; Filippenko, A. V. (2008-04-01). "Supernova 2008bv in UGC 4653". Central Bureau Electronic Telegrams. 1345: 1. Bibcode:2008CBET.1345....1L.
- ^ "Bright Supernovae - 2008". www.rochesterastronomy.org. Retrieved 2024-04-21.
- ^ "SN 2008bv". w.astro.berkeley.edu. Retrieved 2024-04-21.
