UGC 4798
| UGC 4798 | |
|---|---|
 UGC 4798 imaged by Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Lynx |
| Right ascension | 09h 08m 42.6378s[1] |
| Declination | +44° 48′ 38.394″[1] |
| Redshift | 0.026739±0.0000123[1] |
| Heliocentric radial velocity | 8,016±4 km/s[1] |
| Distance | 394.9 ± 27.7 Mly (121.07 ± 8.48 Mpc)[1] |
| Apparent magnitude (V) | 15.0g[1] |
| Characteristics | |
| Type | SAcd[1] |
| Size | ~127,100 ly (38.96 kpc) (estimated)[1] |
| Apparent size (V) | 0.92′ × 0.66′[1] |
| Other designations | |
| 2MASX J09084267+4448379, MCG +08-17-038, PGC 025726, CGCG 238-013[1] | |
UGC 4798 is a spiral galaxy in the constellation of Lynx. Its velocity with respect to the cosmic microwave background is 8,209±14 km/s, which corresponds to a Hubble distance of 394.9 ± 27.7 Mly (121.07 ± 8.48 Mpc).[1]. The first known reference to this galaxy comes from Part 1 of the Morphological Catalogue of Galaxies, published in 1962, where it is listed as MCG +08-17-038.[2]
Supernovae
[edit]Five supernovae have been observed in UGC 4798:
- SN 2005mf (Type Ic, mag. 17.4) was discovered by the THCA Supernova Survey on 25 December 2005.[3][4]
- SN 2013V (Type Ia, mag. 17.8) was discovered by T. Crowley, Jack Newton, and Tim Puckett on 6 January 2013.[5][6]
- PSN J09084248+4448132 (Type Ia, mag. 15.8) was discovered by the Catalina Real-time Transient Survey and Stan Howerton on 26 October 2014.[7][8]
- SN 2019cad (Type Ic, mag. 18.75) was discovered by the Zwicky Transient Facility on 17 March 2019.[9] This supernova was double-peaked and resembled SN 2005bf.[10]
- SN 2025ane (Type II, mag. 18.2563) was discovered by the Zwicky Transient Facility on 31 January 2025.[11]
References
[edit]- 1 2 3 4 5 6 7 8 9 10 11 "Results for object UGC 04798". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 8 December 2025.
- ↑ Vorontsov-Vel'Yaminov, B. A.; Arkhipova, V. P. (1962). "Morphological catalogue of galaxies. Part 1". Morphological Catalogue of Galaxies. C01. Bibcode:1962MCG...C01....0V.
- ↑ Newton, J.; Puckett, T. (2005). "Supernovae 2005mf and 2005mg". International Astronomical Union Circular (8648): 2. Bibcode:2005IAUC.8648....2N.
- ↑ "SN 2005mf". Transient Name Server. IAU. Retrieved 8 December 2025.
- ↑ Crowley, T.; Newton, J.; Puckett, T.; Elenin, L.; Molotov, I.; Tomasella, L.; Benetti, S.; Cappellaro, E.; Pastorello, A.; Turatto, M.; Ochner, P.; Elias-Rosa, N.; Morales-Garoffolo, A. (2013). "Supernova 2013V in UGC 4798 = PSN J09084154+4448496". Central Bureau Electronic Telegrams (3411): 1. Bibcode:2013CBET.3411....1C.
- ↑ "SN 2013V". Transient Name Server. IAU. Retrieved 8 December 2025.
- ↑ Bishop, David. "Bright Supernovae - 2014 - Entry for PSN J09084248+4448132". Rochester Astronomy. Retrieved 8 December 2025.
- ↑ Elias-Rosa, N.; Cappellaro, E.; Benetti, S.; Milan, M.; Miluzio, M.; Ochner, P.; Pastorello, A.; Tartaglia, L.; Terreran, G.; Tomasella, L.; Turatto, M.; Morales-Garoffolo, A.; Huang, F. (2014). "Asiago spectroscopic classification of three SNe". The Astronomer's Telegram. 6628: 1. Bibcode:2014ATel.6628....1E.
- ↑ "SN 2019cad". Transient Name Server. IAU. Retrieved 8 December 2025.
- ↑ Gutiérrez, C. P.; Bersten, M. C.; Orellana, M.; Pastorello, A.; Ertini, K.; Folatelli, G.; Pignata, G.; Anderson, J. P.; Smartt, S.; Sullivan, M.; Pursiainen, M.; Inserra, C.; Elias-Rosa, N.; Fraser, M.; Kankare, E.; Moran, S.; Reguitti, A.; Reynolds, T. M.; Stritzinger, M.; Burke, J.; Frohmaier, C.; Galbany, L.; Hiramatsu, D.; Howell, D. A.; Kuncarayakti, H.; Mattila, S.; Müller-Bravo, T.; Pellegrino, C.; Smith, M. (2021). "The double-peaked Type Ic supernova 2019cad: Another SN 2005bf-like object". Monthly Notices of the Royal Astronomical Society. 504 (4): 4907–4922. arXiv:2104.03723. doi:10.1093/mnras/stab1009.
- ↑ "SN 2025ane". Transient Name Server. IAU. Retrieved 8 December 2025.
External links
[edit]- UGC 4798 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
