IC 5145
| IC 5145 | |
|---|---|
| SDSS image of IC 5145 | |
| Observation data (J2000 epoch) | |
| Constellation | Pegasus |
| Right ascension | 21h 54m 23.06s |
| Declination | +15° 09′ 24.6″ |
| Redshift | 0.024594 |
| Heliocentric radial velocity | 7,373 km/s |
| Distance | 356 Mly (109.2 Mpc) |
| Apparent magnitude (V) | 14.30 |
| Surface brightness | 13.8 arcmin |
| Characteristics | |
| Type | Sab |
| Size | 1.6 x 0.9 arcmin |
| Other designations | |
| UGC 11844, CGCG 427-041, PGC 67619, NSA 149423, WBL 674-003, MCG +02-55-028, 2MASX J21542304+1509244, 2MASS J21542306+1509249, SDSS J215423.07+150924.9, LEDA 67619 | |
IC 5145 is a type Sab spiral galaxy [1] located in the constellation Pegasus.[2] [3] It is located 356 million light-years from the Solar System [4] and was discovered by Edward Emerson Barnard, although the year he discovered it is unknown.[5]
The luminosity class of IC 5145 is I-II and it has a broad H II region.[4] Its dimensions measure 1.60 x 0.9 arcmin.[6]
Supernovae
[edit ]Six supernovae have been discovered in IC 5145 so far: SN 2002dn, SN 2003hy, SN 2010iq, PSN J21542359+1509224, SN 2020pkj, and SN 2022lfa.
SN 2002dn
SN 2002dn[7] was discovered in IC 5145 by astronomer W. D. Li from University of California at Berkeley via unfiltered KAIT CCD images taken on June 15 and June 17, 2002.[8] It was located 8".8 west and 18".3 north of the nucleus.[9] A further inspection done by A. V. Filippenko, R. Chornock and R. J. Foley, using the Shane 3-m reflector at Lick Observatory confirmed SN 2002dn was a Type Ic supernova which resembled SN 1987m.[8] [7]
SN 2003hy
SN 2003hy[10] was discovered by British amateur astronomer, Tom Boles from Coddenham, England on September 14, through unfiltered CCD images using a 0.35-m reflector as part of the course done by U.K. Nova/Supernova Patrol.[11] Surprising, SN 2003hy was also discovered by another amateur astronomer, Mark Armstrong who saw it on the same unfiltered CCD images and via a 0.35m reflector.[11] It had a magnitude of 16.6[10] and was located 5".5 west and 12".5 north of the nucleus.[12] The supernova was Type IIn.[10]
A 14-minute exposure of SN 2003hy taken on December 28, 2003, shows it is much dimmer than 19.4 magnitude, which the dimmest stars are magnitude 20.[13]
SN 2010iq
Lick Observatory Supernova Search discovered SN 2010iq on October 11, 2010.[14] It was reported by A. Narla, S. B. Cenko, W. Li and A. V. Filippenko from University of California, Berkeley through unfiltered CCD images.[15] It was located 2".8 east and 4".4 south of the nucleus with a magnitude of 18.2.[14] This supernova was Type Ic.[14]
PSN J21542359+1509224
PSN J21542359+1509224 was discovered on 13 May 2014 by Bin Wang and Xing Gao.[16] It was located 5".3 east and 0".9 south of the nucleus with a magnitude of 18.3. This supernova had an unknown type.[16]
SN 2020pkj
SN 2020pkj (type Ia, mag. 19.2) was discovered on 15 July 2020 by ZTF.[17]
SN 2022lfa
SN 2022lfa[18] was discovered on May 28, 2022, by Zwicky Transient Facility (ZTF) through Palomar 1.2m Oschin telescope on the behalf of K. De from Caltech.[19] On June 28, 2022, astronomers confirmed that SN 2022lfa is a Type Ic supernova via a spectrum obtained on MJD 59755.43 using the 3-m Shane telescope at Lick Observatory.[20]
References
[edit ]- ^ "HyperLeda -object description". atlas.obs-hp.fr. Retrieved 2024年05月06日.
- ^ Ford, Dominic. "IC5145 (Galaxy)". In-The-Sky.org. Retrieved 2024年05月06日.
- ^ Astronomy, Go. "IC 5145 | galaxy in Pegasus | IC List | GO ASTRONOMY". Go-Astronomy.com. Retrieved 2024年05月06日.
- ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024年05月06日.
- ^ "Index Catalog Objects: IC 5100 - 5149". cseligman.com. Retrieved 2024年05月06日.
- ^ "Revised IC Data for IC 5145". spider.seds.org. Retrieved 2024年05月06日.
- ^ a b "SN 2002dn | Transient Name Server". www.wis-tns.org. Retrieved 2024年05月06日.
- ^ a b Li, W. D.; Filippenko, A. V.; Chornock, R.; Foley, R. J. (2002年06月01日). "Supernova 2002dn in IC 5145". International Astronomical Union Circular (7922): 1. Bibcode:2002IAUC.7922....1L. ISSN 0081-0304.
- ^ "SN 2002dn". w.astro.berkeley.edu. Retrieved 2024年05月06日.
- ^ a b c "SN 2003hy | Transient Name Server". www.wis-tns.org. Retrieved 2024年05月06日.
- ^ a b Boles, T.; Armstrong, M. (2003年09月01日). "Supernova 2003hy in IC 5145". International Astronomical Union Circular (8200): 1. Bibcode:2003IAUC.8200....1B. ISSN 0081-0304.
- ^ "Bright Supernovae - 2003". www.rochesterastronomy.org. Retrieved 2024年05月06日.
- ^ "SN 2003hy in IC 5145". www.kopernik.org. Retrieved 2024年05月06日.
- ^ a b c dbishopx@gmail.com. "Bright Supernovae - 2010". www.rochesterastronomy.org. Retrieved 2024年05月06日.
- ^ Narla, A.; Cenko, S. B.; Li, W.; Filippenko, A. V. (2010年10月01日). "Supernova 2010iq in IC 5145". Central Bureau Electronic Telegrams. 2493: 1. Bibcode:2010CBET.2493....1N.
- ^ a b "Bright Supernovae - 2014". www.rochesterastronomy.org. Retrieved 2024年05月06日.
- ^ "SN 2020pkj". Transient Name Server. IAU . Retrieved 16 August 2024.
- ^ "SN 2022lfa | Transient Name Server". www.wis-tns.org. Retrieved 2024年05月06日.
- ^ "Discovery certificate for object 2022lfa | Transient Name Server". www.wis-tns.org. Retrieved 2024年05月06日.
- ^ "Classification certificate for object 2022lfa | Transient Name Server". www.wis-tns.org. Retrieved 2024年05月06日.