Astronomy:NGC 4309
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Short description: Galaxy in the constellation Virgo
NGC 4309 | |
---|---|
SDSS image of NGC 4309 | |
Observation data (J2000 epoch) | |
Constellation | Virgo[1] |
Right ascension | 12h 22m 12.4s[2] |
Declination | 07° 08′ 40″[2] |
Redshift | 0.002899[2] |
Helio radial velocity | 869 km/s[2] |
Distance | 54 Mly (16.6 Mpc)[2] |
Group or cluster | Virgo Cluster |
Apparent magnitude (V) | 13.6[2] |
Characteristics | |
Type | SAB0^+(r)[2] |
Size | ~62,000 ly (19 kpc) (estimated)[2] |
Apparent size (V) | 4.99 x 0.79[2] |
Other designations | |
UGC 7435, PGC 40051, VCC 0534, MCG +01-32-025[2] |
NGC 4309 is a lenticular galaxy located about 55 million light-years away[3] in the constellation Virgo. The galaxy was discovered by astronomer Christian Peters in 1881[4] and is a member of the Virgo Cluster.[5][6]
NGC 4309 is classified as an AGN[7] and has undergone ram-pressure stripping.[8]
Globular clusters
Within a distance of 160,000 ly (50 kpc) from NGC 4309 exists a population of 162 globular clusters that surround the galaxy.[9]
See also
References
- ↑ R. W. Sinnott, ed (1988). The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation and Cambridge University Press. ISBN 978-0-933346-51-2.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 2.8 2.9 "NASA/IPAC Extragalactic Database". Results for NGC 4309. http://nedwww.ipac.caltech.edu/.
- ↑ "Your NED Search Results". https://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+4309&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES.
- ↑ "New General Catalog Objects: NGC 4300 - 4349". https://cseligman.com/text/atlas/ngc43.htm#4309.
- ↑ Binggeli, B.; Sandage, A.; Tammann, G. A. (1985-09-01). "Studies of the Virgo Cluster. II - A catalog of 2096 galaxies in the Virgo Cluster area.". The Astronomical Journal 90: 1681–1759. doi:10.1086/113874. ISSN 0004-6256. Bibcode: 1985AJ.....90.1681B.
- ↑ "Detailed Object Classifications". https://ned.ipac.caltech.edu/cgi-bin/NEDatt?objname=NGC+4309.
- ↑ Gavazzi, G.; Fumagalli, M.; Fossati, M.; Galardo, V.; Grossetti, F.; Boselli, A.; Giovanelli, R.; Haynes, M. P. (2013-05-01). "Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. II. Star formation properties of galaxies in the Virgo cluster and surroundings". Astronomy and Astrophysics 553: A89. doi:10.1051/0004-6361/201218789. ISSN 0004-6361. Bibcode: 2013A&A...553A..89G.
- ↑ Köppen, J; Jáchym, P; Taylor, R; Palouš, J (2018-10-01). "Ram pressure stripping made easy: an analytical approach" (in en). Monthly Notices of the Royal Astronomical Society 479 (4): 4367–4390. doi:10.1093/mnras/sty1610. ISSN 0035-8711. Bibcode: 2018MNRAS.479.4367K.
- ↑ Zaritsky, Dennis; Aravena, Manuel; Athanassoula, E.; Bosma, Albert; Comerón, Sébastien; Elmegreen, Bruce G.; Erroz-Ferrer, Santiago; Gadotti, Dimitri A. et al. (2015-01-27). "Globular Cluster Populations: First Results from S4G Early-Type Galaxies". The Astrophysical Journal 799 (2): 159. doi:10.1088/0004-637X/799/2/159. ISSN 1538-4357. Bibcode: 2015ApJ...799..159Z.
External links
- NGC 4309 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Original source: https://en.wikipedia.org/wiki/NGC 4309.
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