NGC 5247
| NGC 5247 | |
|---|---|
 Image of NGC 5247 made in infrared light with the HAWK-I camera on ESO's Very Large Telescope at Paranal Observatory. | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 13h 38m 03.040s[1] |
| Declination | –17° 53′ 02.50″[1] |
| Redshift | 0.004520[2] |
| Heliocentric radial velocity | +1,357[3] km/s |
| Distance | 60.34 Mly (18.50 Mpc)[3] |
| Apparent magnitude (V) | 10.5[2] |
| Characteristics | |
| Type | SA(s)bc[2] |
| Apparent size (V) | 5′.6 × 4′.9[2] |
| Other designations | |
| UGCA 368,[2] PGC 48171[2] | |
NGC 5247 is a face-on unbarred spiral galaxy located some 60[3] million light years away in the constellation Virgo. It is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.[4] This is a grand design spiral galaxy that displays no indications of distortion caused by interaction with other galaxies.[5] It has two spiral arms that bifurcate after wrapping halfway around the nucleus.[6] The disk is estimated to be 4.9 ± 2.0 kly (1.5 ± 0.6 kpc) in thickness and it is inclined by roughly 28° to the line of sight.[5]
Supernovae
[edit]Two supernovae have been observed in NGC 5247:
- PSN J13375721-1754272 (type II-P, mag. 15.6) was discovered by the Catalina Real-time Transient Survey on 24 July 2012.[7]
- SN 2016C (type IIP, mag. 15.7) was discovered by Masakatsu Aoki on 3 January 2016.[8]
References
[edit]- ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
- ^ a b c d e f "NASA/IPAC Extragalactic Database". Results for NGC 5247. Retrieved 2007-04-03.
- ^ a b c Crook, Aidan C.; et al. (February 2007), "Groups of Galaxies in the Two Micron All Sky Redshift Survey", The Astrophysical Journal, 655 (2): 790–813, arXiv:astro-ph/0610732, Bibcode:2007ApJ...655..790C, doi:10.1086/510201, S2CID 11672751.
- ^ "The Virgo III Groups". Atlas of the Universe. Retrieved 2010-11-27.
- ^ a b Khoperskov, S. A.; et al. (December 2012), "Global gravitationally organized spiral waves and the structure of NGC 5247", The Astrophysical Journal, 427 (3): 1983–1993, arXiv:1209.2879, Bibcode:2012MNRAS.427.1983K, doi:10.1111/j.1365-2966.2012.22031.x, S2CID 119186508.
- ^ Patsis, P. A.; et al. (July 1997), "Interarm features in gaseous models of spiral galaxies", Astronomy and Astrophysics, 323: 762–774, Bibcode:1997A&A...323..762P.
- ^ Bishop, David. "Bright Supernovae - 2012 - Entry for PSNJ13375721-1754272". Rochester Astronomy. Retrieved 11 December 2024.
- ^ "SN 2016C". Transient Name Server. IAU. Retrieved 11 December 2024.
External links
[edit]
Media related to NGC 5247 at Wikimedia Commons- NGC 5247 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
 | This spiral galaxy article is a stub. You can help Wikipedia by expanding it. |