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NGC 5247

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)
ConstellationVirgo
Right ascension13h 38m 03.040s[1]
Declination–17° 53′ 02.50″[1]
Redshift0.004520[2]
Heliocentric radial velocity+1,357[3] km/s
Distance60.34 Mly
(18.50 Mpc)[3]
Apparent magnitude (V)10.5[2]
Characteristics
TypeSA(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]

One supernova has been observed in NGC 5247: SN 2016C (type IIP, mag. 15.7).[7]

NGC 5247 in ultraviolet by GALEX

References

  1. ^ 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.
  2. ^ a b c d e f "NASA/IPAC Extragalactic Database". Results for NGC 5247. Retrieved 2007-04-03.
  3. ^ 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.
  4. ^ "The Virgo III Groups". Atlas of the Universe. Retrieved 2010-11-27.
  5. ^ 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.
  6. ^ 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.
  7. ^ Transient Name Server entry for SN 2016C. Retrieved 23 March 2023.



Quelle: https://en.wikipedia.org/wiki/NGC_5247