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NGC 4527

Coordinates:Sky map12h 34m 08.466s, +02° 39′ 14.414″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Virgo
NGC 4527
NGC 4527 imaged bySDSS
Observation data (J2000epoch)
ConstellationVirgo
Right ascension12h 34m 08.466s[1]
Declination+02° 39′ 14.414″[1]
Redshift0.005791[1]
Heliocentric radial velocity1736 ± 1 km/s[1]
Distance48.9Mly
Apparent magnitude (V)11.4[1]
Characteristics
TypeSAB(s)bc[1]
Size~104,100 ly (31.92 kpc) (estimated)[1]
Apparent size (V)6.2′ × 2.1′[1]
Other designations
IRAS 12315+0255,UGC 7721,MCG +01-32-101,PGC 41789,CGCG 042-156[1]

NGC 4527 is aspiral galaxy in theconstellationVirgo. It was discovered by German-British astronomerWilliam Herschel on 23 February 1784.[2]

NGC 4527 is a member of theM61 Group of galaxies, which is a member of theVirgo II Groups, a series of galaxies andgalaxy clusters strung out from the southern edge of theVirgo Supercluster.[3]

Characteristics

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NGC 4527 is anintermediate spiral galaxy similar to theAndromeda Galaxy[4] and is located at a distance not well determined, but usually is considered to be an outlying member of theVirgo Cluster of galaxies,[5] being placed within the subcluster known asS Cloud.[6]

Unlike the Andromeda Galaxy, NGC 4527 is also astarburst galaxy, with 2.5 billionsolar masses ofmolecular hydrogen concentrated within its innermost regions.[7] However said starburst is still weak and seems to be on its earliest phases.[7]

Supernovae

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Threesupernovae have been observed in NGC 4527:

  • SN 1915A (type unknown, mag. 15.5) was discovered byHeber Curtis on 20 March 1915.[8][9][10]
  • SN 1991T (Type Ia-pec, mag. 13) was discovered by Stephen Knight on 13 April 1991, and independently reported byRobert Evans, Mirko Villi, Giancarlo Cortini, and Wayne Johnson.[11][12] This supernova has been studied extensively as a peculiar and overluminous Type Ia, and is now used as a template, with similar events being classified asType Ia-91T-like.[13][14]
  • SN 2004gn (Type Ic, mag. 16.6) was discovered by theLick Observatory Supernova Search (LOSS) on 1 December 2004.[15][16][17]
NGC 4527 imaged by theHubble Space Telescope

See also

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References

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  1. ^abcdefghi"Results for NGC 4527".NASA/IPAC Extragalactic Database. Retrieved2013-10-12.
  2. ^Seligman, Courtney."New General Catalogue Objects: NGC 4527".Celestial Atlas. Retrieved6 December 2024.
  3. ^"The Virgo III Groups".Atlas of the Universe. Retrieved2010-11-27.
  4. ^"Best of AOP: NGC 4527". NOAO. Retrieved2013-10-12.
  5. ^"Notes for object NGC 4527". NASA-IPAC Extragalactic Database. Retrieved2013-10-12.
  6. ^"Galaxy On Line Database Milano Network (GOLDMine)". Retrieved2012-08-06.
  7. ^abShibatsuka, T.; Matsushita, S.; Kohno, K.; Kawabe, R. (2003)."Multi-Line Observations of Molecular Gas in the Central Region of the Low Star-Formation EfficiencyStarburst Galaxy NGC 4527".Publications of the Astronomical Society of Japan.55 (1):87–101.Bibcode:2003PASJ...55...87S.doi:10.1093/pasj/55.1.87.
  8. ^"SN 1915A".Transient Name Server.IAU. Retrieved6 December 2024.
  9. ^Central Bureau for Astronomical Telegrams list of Supernovae. Retrieved 28 March 2023.
  10. ^Shapley, Harlow (1917). "A Faint Nova in the Nebula of Andromeda".Publications of the Astronomical Society of the Pacific.29 (171):213–217.Bibcode:1917PASP...29Q.213S.doi:10.1086/122669.
  11. ^Waagen, E.; Evans, R. O.; Villi, M.; Cortini, G.; Johnson, W.; McNaught, R. H.; Mueller, J.; Cappellaro, E.; Cutispoto, G.; La Franca, F.; Goldschmidt, C.; Kirshner, R. P.; Peters, J. (1991). "Supernova 1991T in NGC 4527".International Astronomical Union Circular (5239): 1.Bibcode:1991IAUC.5239....1W.
  12. ^"SN 1991T".Transient Name Server.IAU. Retrieved6 December 2024.
  13. ^Lira, P.; Suntzeff, Nicholas B.; Phillips, M. M.; Hamuy, Mario; Maza, José; Schommer, R. A.; Smith, R. C.; Wells, Lisa A.; Avilés, R.; Baldwin, J. A.; Elias, J. H.; González, L.; Layden, A.; Navarrete, M.; Ugarte, P.; Walker, Alistair R.; Williger, Gerard M.; Baganoff, F. K.; Crotts, Arlin P. S.; Rich, R. Michael; Tyson, N. D.; Dey, A.; Guhathakurta, P.; Hibbard, J.; Kim, Y. -C.; Rehner, Daniel M.; Siciliano, E.; Roth, Joshua; Seitzer, Patrick; Williams, T. B. (1998). "Optical Light Curves of the Type IA Supernovae SN 1990N and SN 1991T".The Astronomical Journal.115 (1): 234.arXiv:astro-ph/9709262.Bibcode:1998AJ....115..234L.doi:10.1086/300175.
  14. ^Sasdelli, Michele; Mazzali, P. A.; Pian, E.; Nomoto, K.; Hachinger, S.; Cappellaro, E.; Benetti, S. (2014)."Abundance stratification in Type Ia supernovae - IV. The luminous, peculiar SN 1991T".Monthly Notices of the Royal Astronomical Society.445 (1): 711.arXiv:1409.0116.Bibcode:2014MNRAS.445..711S.doi:10.1093/mnras/stu1777.
  15. ^"SN 2004gn".Transient Name Server.IAU. Retrieved6 December 2024.
  16. ^Li, W. (2004). "Supernovae 2004gn and 2004go".International Astronomical Union Circular (8448): 2.Bibcode:2004IAUC.8448....2L.
  17. ^Bishop, David."Bright Supernovae - 2004, entry for SN 2004gn".Rochester Astronomy. Retrieved25 November 2024.

External links

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  • Media related toNGC 4527 at Wikimedia Commons
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