UGC 4457
| UGC 4457 | |
|---|---|
 Hubble Space Telescope image of UGC 4457 | |
| Observation data | |
| Constellation | Cancer |
| Right ascension | 127.9 degrees |
| Redshift | 0.03718 0.00001 |
| Heliocentric radial velocity | 11,162 km/s |
| Distance | 500 Mly (153.3 Mpc) |
| Apparent magnitude (V) | 15.131 |
| Notable features | Interacting 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
- ^ a b c "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-19.
- ^ Guide, Universe (2022-07-03). "UGC 4457 Facts". Universe Guide. Retrieved 2024-04-19.
- ^ a b "Principal Galaxy Catalog (PGC) Objects 23500 to 23999". cseligman.com. Retrieved 2024-04-19.
- ^ "1983MNRAS.204..909R Page 909". adsabs.harvard.edu. Bibcode:1983MNRAS.204..909R. Retrieved 2024-04-21.
- ^ "Arp 58 - Astronomy Magazine - Interactive Star Charts, Planets, Meteors, Comets, Telescopes". cs.astronomy.com. Retrieved 2024-04-19.
- ^ 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.
