UGC 4457

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UGC 4457
Hubble Space Telescope image of UGC 4457
Observation data
ConstellationCancer
Right ascension127.9 degree
Redshift0.03718 0.00001
Heliocentric radial velocity11,162 km/s
Distance500 Mly (153.3 Mpc)
Apparent magnitude (V)15.131
Notable featuresInteracting galaxy
Other designations
UGC 4457 PGC 23935, Arp 58, IRAS 08290+1922, MCG +03-22-017, VV 413, LEDA 23935, Z 89-40

UGC 4457 known as PGC 23935, is a barred spiral galaxy, containing an active galactic nucleus in the Cancer constellation.[1][2][3] It is located 500 million light-years away from the solar system[3] and has a diameter of 290,000 light-years,[1] making it slightly more massive compared to the Milky Way.[4] The galaxy is moving away at a speed of 11,162 kilometers per second.[1]

UGC 4457 is interacting with the compact galaxy, PGC 23937. Together, they form Arp 58 and are classified under spiral galaxies that have small companions with high surface brightness.[5] UGC 4457 shows disturbed spiral arms, indicating signs of velocity disturbance levels and regions of scattered ionized gas, typically normal for interacting galaxies. A faint spiral bridge can be seen thus representing the remains of an older mode of spiral waves.[6]

References[edit]

  1. ^ a b c "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-19.
  2. ^ Guide, Universe (2022-07-03). "UGC 4457 Facts". Universe Guide. Retrieved 2024-04-19.
  3. ^ a b "Principal Galaxy Catalog (PGC) Objects 23500 to 23999". cseligman.com. Retrieved 2024-04-19.
  4. ^ "1983MNRAS.204..909R Page 909". adsabs.harvard.edu. Bibcode:1983MNRAS.204..909R. Retrieved 2024-04-21.
  5. ^ "Arp 58 - Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets, Telescopes". cs.astronomy.com. Retrieved 2024-04-19.
  6. ^ Zasov, Anatoly V.; Saburova, Anna S.; Egorov, Oleg V.; Dodonov, Sergei N. (2019-06-01). "Spectral observations of the systems with the disturbed spiral arms: Arp 42, Arp 82, and Arp 58". Monthly Notices of the Royal Astronomical Society. 486 (2): 2604–2617. arXiv:1904.03150. Bibcode:2019MNRAS.486.2604Z. doi:10.1093/mnras/stz1025. ISSN 0035-8711.