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NGC 5668

Coordinates:Sky map14h 33m 24.331s, +04° 27′ 01.75″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Virgo
NGC 5668
A spiral galaxy, seen up close and face-on. It is coloured yellow and glowing brightly at the oval-shaped centre, showing older and cooler stars, and it becomes bluer out to the edge of the disc where the stars are younger and hotter. It has a number of somewhat patchy spiral arms curling around, with sparkling areas where stars form. The black background can just be seen at the corners.
NGC 5668 imaged by theHubble Space Telescope
Observation data (J2000epoch)
ConstellationVirgo
Right ascension14h 33m 24.331s[1]
Declination+04° 27′ 01.75″[1]
Redshift0.005280
Heliocentric radial velocity1,582 ± 5[2]km/s
Distance80.9 ± 5.5 millionlight years(24.8 ± 1.7Mpc)[2]
Group orclusterNGC 5638 Group, NGC 5746 Group, Virgo III Groups
Characteristics
TypeSA(s)d[2]
Mass5.7×1010[2] M
Size~48,400 ly (14.84 kpc) (estimated)
Apparent size (V)3.0′ × 3.0′
Other designations
IRAS 14309+0440,UGC 9363,MCG +01-37-028,PGC 52018,CGCG 047-090[3]

NGC 5668 is a nearly face-onspiral galaxy, visualmagnitude about 11.5,[4] located about 81[2] millionlight years away in theconstellationVirgo. It was discovered on 29 April 1786 byWilliam Herschel.[4]

NGC 5668 is a member of theNGC 5638 Group of galaxies, itself one of theVirgo III Groups strung out to the east of theVirgo Supercluster of galaxies.[5] In addition, A.M. Garcia listed NGC 5668 in the 31 memberNGC 5746 galaxy group (also known asLGG 386).[6]

As seen from theEarth, it is inclined by an angle of 18° to theline of sight along aposition angle of 145°. Themorphological classification in theDe Vaucouleurs system is SA(s)d,[2] indicating a pure spiral structure with loosely wound arms.[7] However, optical images of the galaxy indicate the presence of a weak bar structure spanning an angle of 12″ across the nucleus. There is adwarf galaxy located around 650×10^3 ly (200 kpc) to the southeast of NGC 5668, and the two may be gravitationally interacting.[2]

Supernovae

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Threesupernovae have been observed in this galaxy:

  • SN 1952G (type unknown, mag. 17.9) was discovered byFritz Zwicky on 18 April 1952.[8][9]
  • SN 1954B (Type Ia, mag. 12.3) was discovered byPaul Wild on 4 May 1954.[10] [Note: Some sources incorrectly list the discovery date as 27 April 1954.][11]
  • SN 2004G (Type II, mag. 17.2) was discovered byReiki Kushida on 19 January 2004.[12][13][14] It was initially imaged at 43" to the west and 12".5 south of the galaxy core.[13]

High velocity clouds ofneutral hydrogen have been observed in NGC 5668, which may have their origin in supernova explosions and strongstellar winds.[15]

Gallery

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  • NGC 5668 (SDSS DR14)
    NGC 5668 (SDSS DR14)
  • GALEX image of NGC 5668
    GALEX image of NGC 5668

See also

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References

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  1. ^abSkrutskie, 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. ^abcdefgR. A., Marino; et al. (July 2012), "Integral Field Spectroscopy and Multi-wavelength Imaging of the nearby Spiral Galaxy NGC 5668: An Unusual Flattening in Metallicity Gradient",The Astrophysical Journal,754 (1): 61,arXiv:1205.5051,Bibcode:2012ApJ...754...61M,doi:10.1088/0004-637X/754/1/61,S2CID 2243509.
  3. ^"NGC 5668 -- Galaxy",SIMBAD Astronomical Database,Centre de Données astronomiques de Strasbourg, retrieved2013-07-11.
  4. ^ab"New General Catalog Objects: NGC 5650 - 5699".cseligman.com. Retrieved2021-03-12.
  5. ^"The Virgo III Groups".Atlas of the Universe. Retrieved2010-11-27.
  6. ^Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups".Astronomy and Astrophysics Supplement Series.100: 47.Bibcode:1993A&AS..100...47G.
  7. ^Buta, Ronald J.; et al. (2007),Atlas of Galaxies,Cambridge University Press, pp. 13–17,ISBN 978-0521820486.
  8. ^"SN 1952G".Transient Name Server.IAU. Retrieved7 September 2024.
  9. ^Kowal, C. T.; Zwicky, F.; Sargent, W. L. W.; Searle, L. (1974)."The 1973 Palomar Supernova Search".Publications of the Astronomical Society of the Pacific.86 (512): 516.Bibcode:1974PASP...86..516K.doi:10.1086/129639.
  10. ^Wild, Paul (1960)."Light Curves of the Supernovae of 1954".Publications of the Astronomical Society of the Pacific.72 (425): 97.Bibcode:1960PASP...72...97W.doi:10.1086/127488.
  11. ^"SN 1954B".Transient Name Server.IAU. Retrieved7 September 2024.
  12. ^"SN 2004G".Transient Name Server.IAU. Retrieved7 September 2024.
  13. ^abNakano, S.; et al. (2004), "Supernova 2004G in NGC 5668",IAU Circular (8272): 1,Bibcode:2004IAUC.8272....1N.
  14. ^Elias-Rosa, N.; et al. (2004), "Supernova 2004G in NGC 5668",IAU Circular (8273): 2,Bibcode:2004IAUC.8273....2E.
  15. ^Jiménez-Vicente, J.; Battaner, E. (June 2000), "Vertical motions in the disk of NGC 5668 as seen with optical Fabry-Perot spectroscopy",Astronomy and Astrophysics,358:812–818,arXiv:astro-ph/0004295,Bibcode:2000A&A...358..812J.

External links

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  • Media related toNGC 5668 at Wikimedia Commons


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