Astronomy:UGC 4798
From HandWiki
| 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] |
| Helio 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 | |
| MCG+08-17-038, PGC 025726[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
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
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 "Results for object UGC 04798". NASA and Caltech. https://ned.ipac.caltech.edu/byname?objname=UGC+04798.
- ↑ 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. http://www.cbat.eps.harvard.edu/iauc/08600/08648.html#Item2.
- ↑ "SN 2005mf". IAU. https://www.wis-tns.org/object/2005mf.
- ↑ Crowley, T.; Newton, J.; Puckett, T.; Elenin, L.; Molotov, I.; Tomasella, L.; Benetti, S.; Cappellaro, E. et al. (2013). "Supernova 2013V in UGC 4798 = PSN J09084154+4448496". Central Bureau Electronic Telegrams (3411): 1. Bibcode: 2013CBET.3411....1C.
- ↑ "SN 2013V". IAU. https://www.wis-tns.org/object/2013V.
- ↑ Bishop, David. "Bright Supernovae - 2014 - Entry for PSN J09084248+4448132". https://www.rochesterastronomy.org/sn2014/index.html#PSNJ09084248+4448132.
- ↑ Elias-Rosa, N.; Cappellaro, E.; Benetti, S.; Milan, M.; Miluzio, M.; Ochner, P.; Pastorello, A.; Tartaglia, L. et al. (2014). "Asiago spectroscopic classification of three SNe". The Astronomer's Telegram 6628: 1. Bibcode: 2014ATel.6628....1E. https://www.astronomerstelegram.org/?read=6628.
- ↑ "SN 2019cad". IAU. https://www.wis-tns.org/object/2019cad.
- ↑ Gutiérrez, C. P.; Bersten, M. C.; Orellana, M.; Pastorello, A.; Ertini, K.; Folatelli, G.; Pignata, G.; Anderson, J. P. et al. (2021). "The double-peaked Type Ic supernova 2019cad: Another SN 2005bf-like object". Monthly Notices of the Royal Astronomical Society 504 (4): 4907–4922. doi:10.1093/mnras/stab1009.
- ↑ "SN 2025ane". IAU. https://www.wis-tns.org/object/2025ane.
External links
- UGC 4798 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Coordinates:
09h 08m 42.6378s, +44° 48′ 38.394″
