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UGC 4653 information


UGC 4653
Hubble Space Telescope image of UGC 4653
Observation data
ConstellationLynx
Right ascension133.47 degrees
Declination35.14 degrees
Redshift0.056836 0.00143
Heliocentric radial velocity16,748 km/s
Distance763 Mly (233.9 Mpc)
Apparent magnitude (V)13.645 0.004
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

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]

  1. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-21.
  2. ^ a b information@eso.org. "Squabbling Galactic Siblings". www.spacetelescope.org. Retrieved 2024-04-21.
  3. ^ "Halton Arp's Atlas of Peculiar Galaxies". cseligman.com. Retrieved 2024-04-21.
  4. ^ "Arp 195 - Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets, Telescopes". cs.astronomy.com. Retrieved 2024-04-21.
  5. ^ a b Fiorenza, Stephanie; Uzan, Raphael (2019). "A Study of the Nuclear Regions of the Triple Merging System Arp 195". American Astronomical Society Meeting Abstracts #233. 233. Bibcode:2019AAS...23317302F. Retrieved 27 April 2024.

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