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NGC 4333 is a barred spiral galaxy with a ring structure[2] located about 330 million light-years away[3] in the constellation Virgo. It was discovered by astronomer William Herschel on April 13, 1784,[4] who described it as "F, pS, R, bM, 2nd of 3".[5] NGC 4333 is also classified as a LINER galaxy.[6] Despite being listed in the Virgo Cluster catalog as VCC 637, it is not a member of the Virgo Cluster but instead a background galaxy.[7]

NGC 4333
SDSS image of NGC 4333.
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension12h 23m 22.3s[1]
Declination06° 02′ 27″[1]
Redshift0.023406[1]
Helio radial velocity7017 km/s[1]
Distance330 Mly (100 Mpc)[1]
Apparent magnitude (V)14.48[1]
Characteristics
TypeSB(s)ab[1]
Size~110,800 ly (33.96 kpc) (estimated)[1]
Apparent size (V)0.9 x 0.7[1]
Other designations
VCC 0637, PGC 040217, MCG +01-32-034, CGCG 042-065[1]

Nearby galaxies


NGC 4333 forms a pair with the galaxy NGC 4326, known as [T2015] nest 102514,[8][9] in which NGC 4326 is the birghtest member of the pair.[9] Both galaxies are part of the CfA2 Great Wall.[10]


See also





References


  1. "NASA/IPAC Extragalactic Database". Results for NGC 4333. Retrieved 2022-03-02.
  2. "HyperLeda -object description". leda.univ-lyon1.fr. Retrieved 2022-03-02.
  3. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2022-03-03.
  4. "New General Catalog Objects: NGC 4300 - 4349". cseligman.com. Retrieved 2022-02-19.
  5. "NGC/IC Project Restoration Efforts". ngcicproject.observers.org. Retrieved 2022-03-02.
  6. Toba, Y.; Oyabu, S.; Matsuhara, H.; Malkan, M. A.; Gandhi, P.; Nakagawa, T.; Isobe, N.; Shirahata, M.; Oi, N.; Ohyama, Y.; Takita, S. (2014-05-20). "LUMINOSITY AND REDSHIFT DEPENDENCE OF THE COVERING FACTOR OF ACTIVE GALACTIC NUCLEI VIEWED WITH WISE AND SLOAN DIGITAL SKY SURVEY". The Astrophysical Journal. 788 (1): 45. doi:10.1088/0004-637X/788/1/45. ISSN 0004-637X.
  7. Binggeli, B.; Sandage, A.; Tammann, G. A. (September 1985). "Studies of the Virgo Cluster. II - A catalog of 2096 galaxies in the Virgo Cluster area. V - Luminosity functions of Virgo Cluster galaxies". The Astronomical Journal. 90: 1681. doi:10.1086/113874.
  8. "[T2015] nest 10214". simbad.u-strasbg.fr. Retrieved 2022-02-22.
  9. Tully, R. Brent (2015-05-01). "Galaxy Groups: A 2MASS Catalog". The Astronomical Journal. 149: 171. doi:10.1088/0004-6256/149/5/171. ISSN 0004-6256.
  10. Hoffman, G. Lyle; Lewis, B. M.; Salpeter, E. E. (1995-03-01). "The Large-Scale Distribution of Late-Type Galaxies between Virgo and the Great Wall". The Astrophysical Journal. 441: 28. doi:10.1086/175333. ISSN 0004-637X.

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На других языках

[de] NGC 4333

NGC 4333 ist eine Balken-Spiralgalaxie mit aktivem Galaxienkern vom Hubble-Typ SBab im Sternbild Jungfrau nördlich der Ekliptik. Sie ist schätzungsweise 311 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 75.000 Lichtjahren. Die Galaxie wird unter der Katalognummer VVC 637 als Teil des Virgo-Galaxienhaufens gelistet. Im selben Himmelsareal befinden sich u. a. die Galaxien NGC 4326, NGC 4339, NGC 4376, IC 782.
- [en] NGC 4333

[ru] NGC 4333

NGC 4333 (другие обозначения — MCG 1-32-34, ZWG 42.65, VCC 637, NPM1G +06.0337, PGC 40217) — галактика в созвездии Дева.


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