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NGC 4326 is a barred spiral galaxy with a ring[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 "vF, S, R, bM, 1st of 3".[5] It is a large galaxy, with a diameter of around 200,000 ly (61 kpc) making it nearly twice the size of the Milky Way.[3] NGC 4326 is also classified as a LINER galaxy.[6] Despite being listed in the Virgo Cluster catalog as VCC 623, it is not a member of the Virgo Cluster but instead a background galaxy.[7]

NGC 4326
SDSS image of NGC 4326.
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension12h 23m 11.6s[1]
Declination06° 04′ 20″[1]
Redshift0.023756[1]
Helio radial velocity7122 km/s[1]
Distance330 Mly (102 Mpc)[1]
Apparent magnitude (V)14.19[1]
Characteristics
TypeSAB(r)ab+[1]
Size~200,700 ly (61.54 kpc) (estimated)[1]
Apparent size (V)1.5 x 1.1[1]
Other designations
UGC 07454, VCC 0623, PGC 040192, MCG +01-32-033, CGCG 042-064[1]

Nearby Galaxies


NGC 4326 forms a pair with the galaxy NGC 4333, 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 4326. Retrieved 2022-02-21.
  2. "HyperLeda -object description". leda.univ-lyon1.fr. Retrieved 2022-02-22.
  3. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2022-02-22.
  4. "New General Catalog Objects: NGC 4300 - 4349". cseligman.com. Retrieved 2022-02-19.
  5. "NGC/IC Project Restoration Efforts". ngcicproject.observers.org. Retrieved 2022-02-22.
  6. "NGC 4326". simbad.u-strasbg.fr. Retrieved 2022-02-22.
  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.

На других языках

[de] NGC 4326

NGC 4326 ist eine Balken-Spiralgalaxie mit aktivem Galaxienkern vom Hubble-Typ SBab im Sternbild Jungfrau nördlich der Ekliptik. Sie ist schätzungsweise 315 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 130.000 Lichtjahren. Die Galaxie wird unter der Katalognummer VVC 623 als Teil des Virgo-Galaxienhaufens gelistet, ist dafür jedoch zu weit entfernt. Im selben Himmelsareal befinden sich u. a. die Galaxien NGC 4333, NGC 4339, IC 782, IC 3268.
- [en] NGC 4326

[ru] NGC 4326

NGC 4326 (другие обозначения — UGC 7454, MCG 1-32-33, ZWG 42.64, VCC 623, NPM1G +06.0336, PGC 40192) — галактика в созвездии Дева.


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