From Wikipedia, the free encyclopedia
NGC 4320
SDSS image of NGC 4320.
Observation data ( J2000 epoch)
Constellation Virgo
Right ascension12h 22m 57.7s [1]
Declination10° 32′ 54″ [1]
Redshift0.026675 [1]
Heliocentric radial velocity7997 km/s [1]
Distance370  Mly (114  Mpc) [1]
Group or cluster NGC 4325 Group
Apparent magnitude (V)15.3 [1]
Characteristics
TypeS? pec [2]
Size~120,000  ly (38  kpc) (estimated) [1]
Apparent size (V)0.70 x 0.53 [1]
Other designations
UGC 07452, VCC 0599, PGC 040160, MCG +02-32-018 [1]

NGC 4320, is a peculiar galaxy [2] located about 370 million light-years away [3] in the constellation Virgo. It was discovered by astronomer Heinrich d'Arrest on April 15, 1865 [2] and is a member of the NGC 4325 Group. [4] [5] [6]

NGC 4320 appears to be the end result [2] of an interaction [7] and merger of two spiral galaxies. [2]

See also

References

  1. ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 4320. Retrieved 2019-10-13.
  2. ^ a b c d e "New General Catalog Objects: NGC 4300 - 4349". cseligman.com. Retrieved 2019-08-19.
  3. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-10-13.
  4. ^ Helsdon, Stephen F.; Ponman, Trevor J.; O'Sullivan, Ewan; Forbes, Duncan A. (2001-08-01). "X-ray luminosities of galaxies in groups". Monthly Notices of the Royal Astronomical Society. 325 (2): 693–706. arXiv: astro-ph/0103293. Bibcode: 2001MNRAS.325..693H. doi: 10.1046/j.1365-8711.2001.04490.x. hdl: 1959.3/1854. ISSN  0035-8711. S2CID  17732882.
  5. ^ Jeltema, Tesla E.; Binder, Breanna; Mulchaey, John S. (2008-06-01). "The Hot Gas Halos of Galaxies in Groups". The Astrophysical Journal. 679 (2): 1162–1172. arXiv: 0801.2570. Bibcode: 2008ApJ...679.1162J. doi: 10.1086/587508. ISSN  0004-637X. S2CID  18636670.
  6. ^ Ramella, Massimo; Geller, Margaret J.; Pisani, Armando; da Costa, Luiz N. (June 2002). "The UZC-SSRS2 Group Catalog". The Astronomical Journal. 123 (6): 2976–2984. arXiv: astro-ph/0202326. Bibcode: 2002AJ....123.2976R. doi: 10.1086/340357.
  7. ^ Boselli, A.; Boissier, S.; Heinis, S.; Cortese, L.; Ilbert, O.; Hughes, T.; Cucciati, O.; Davies, J.; Ferrarese, L.; Giovanelli, R.; Haynes, M. P. (April 2011). "The GALEX Ultraviolet Virgo Cluster Survey (GUViCS): I. The UV luminosity function of the central 12 sq. deg". Astronomy & Astrophysics. 528: A107. arXiv: 1102.1316. Bibcode: 2011A&A...528A.107B. doi: 10.1051/0004-6361/201016389. ISSN  0004-6361.

External links


From Wikipedia, the free encyclopedia
NGC 4320
SDSS image of NGC 4320.
Observation data ( J2000 epoch)
Constellation Virgo
Right ascension12h 22m 57.7s [1]
Declination10° 32′ 54″ [1]
Redshift0.026675 [1]
Heliocentric radial velocity7997 km/s [1]
Distance370  Mly (114  Mpc) [1]
Group or cluster NGC 4325 Group
Apparent magnitude (V)15.3 [1]
Characteristics
TypeS? pec [2]
Size~120,000  ly (38  kpc) (estimated) [1]
Apparent size (V)0.70 x 0.53 [1]
Other designations
UGC 07452, VCC 0599, PGC 040160, MCG +02-32-018 [1]

NGC 4320, is a peculiar galaxy [2] located about 370 million light-years away [3] in the constellation Virgo. It was discovered by astronomer Heinrich d'Arrest on April 15, 1865 [2] and is a member of the NGC 4325 Group. [4] [5] [6]

NGC 4320 appears to be the end result [2] of an interaction [7] and merger of two spiral galaxies. [2]

See also

References

  1. ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 4320. Retrieved 2019-10-13.
  2. ^ a b c d e "New General Catalog Objects: NGC 4300 - 4349". cseligman.com. Retrieved 2019-08-19.
  3. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-10-13.
  4. ^ Helsdon, Stephen F.; Ponman, Trevor J.; O'Sullivan, Ewan; Forbes, Duncan A. (2001-08-01). "X-ray luminosities of galaxies in groups". Monthly Notices of the Royal Astronomical Society. 325 (2): 693–706. arXiv: astro-ph/0103293. Bibcode: 2001MNRAS.325..693H. doi: 10.1046/j.1365-8711.2001.04490.x. hdl: 1959.3/1854. ISSN  0035-8711. S2CID  17732882.
  5. ^ Jeltema, Tesla E.; Binder, Breanna; Mulchaey, John S. (2008-06-01). "The Hot Gas Halos of Galaxies in Groups". The Astrophysical Journal. 679 (2): 1162–1172. arXiv: 0801.2570. Bibcode: 2008ApJ...679.1162J. doi: 10.1086/587508. ISSN  0004-637X. S2CID  18636670.
  6. ^ Ramella, Massimo; Geller, Margaret J.; Pisani, Armando; da Costa, Luiz N. (June 2002). "The UZC-SSRS2 Group Catalog". The Astronomical Journal. 123 (6): 2976–2984. arXiv: astro-ph/0202326. Bibcode: 2002AJ....123.2976R. doi: 10.1086/340357.
  7. ^ Boselli, A.; Boissier, S.; Heinis, S.; Cortese, L.; Ilbert, O.; Hughes, T.; Cucciati, O.; Davies, J.; Ferrarese, L.; Giovanelli, R.; Haynes, M. P. (April 2011). "The GALEX Ultraviolet Virgo Cluster Survey (GUViCS): I. The UV luminosity function of the central 12 sq. deg". Astronomy & Astrophysics. 528: A107. arXiv: 1102.1316. Bibcode: 2011A&A...528A.107B. doi: 10.1051/0004-6361/201016389. ISSN  0004-6361.

External links



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