IC 629, ESO 501-43, AM 1034-271, IRAS 10346-2718, MCG -4-25-39, PGC 31513[1]
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NGC 3312 is a large[3] and highly inclined[4] spiral galaxy[5] located about 194 million light-years away[6] in the constellation Hydra.[7] The galaxy was discovered by astronomer John Herschel on March 26, 1835. It was later rediscovered by astronomer Guillaume Bigourdan on February 26, 1887. NGC 3312 was later listed and equated with IC 629 because the two objects share essentially the same celestial coordinates.[8][9] NGC 3312 is the largest spiral galaxy[3] in the Hydra Cluster[3][10] and is also classified as a LINER galaxy.[11][4]
^ abcdefghi"NASA/IPAC Extragalactic Database". Results for NGC 3312. Retrieved 2018-05-29.
^König, Michael; Binnewies, Stefan (2017-09-07). The Cambridge Photographic Atlas of Galaxies. Cambridge University Press. ISBN 978-1-107-18948-5.
^ abcHuchtmeier, W. K. (July 1990). "Detection of CO emission in Hydra 1 cluster galaxies". NASA Conference Publication. 3084: 386–388. Bibcode:1990NASCP3084..386H.
^"Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-05-31.
^"NED Query Results for NGC 3312". ned.ipac.caltech.edu. Retrieved 2018-05-31.
^"Revised NGC Data for NGC 3312". spider.seds.org. Retrieved 2018-05-31.
^Gottlieb, Steve. "Astronomy-Mall: Adventures In Deep Space NGC objects 3001–3999". Astronomy-Mall. Retrieved 2018-04-27.
^"New General Catalog Objects: NGC 3300 – 3349". cseligman.com. Retrieved 2018-05-04.
^Richter, O.-G. (February 1989). "The Hydra I cluster of galaxies. V – A catalogue of galaxies in the cluster area". Astronomy and Astrophysics Supplement Series. 77: 237–256. Bibcode:1989A&AS...77..237R.
NGC3312 is a large and highly inclined spiral galaxy located about 194 million light-years away in the constellation Hydra. The galaxy was discovered...
; Jarrett, Thomas H.; Kraan-Korteweg, Renée C. (2022-12-01). "NGC 3314a/b and NGC3312: Ram pressure stripping in Hydra I cluster substructure". Astronomy...
cluster's largest galaxies are elliptical galaxies NGC 3309 and NGC 3311 and the spiral galaxy NGC3312 all having a diameter of about 150,000 light-years...
3312–3330. arXiv:2108.02791. doi:10.1093/mnras/stab2297. "New General Catalog Objects: NGC 200 - 249". Cseligman. Retrieved September 10, 2016. NGC 222...
NGC 290 is an open cluster of stars in the southern constellation of Tucana. This cluster was discovered September 5, 1826, by Scottish astronomer James...
comes from NGC 3309. The radio emission in NGC 3309 may have been triggered by a recent perturbation with the giant spiral galaxy NGC3312. NGC 3309 has...
Astronomical Society. 507 (3): 3312–3330. arXiv:2108.02791. doi:10.1093/mnras/stab2297. Media related to NGC 176 at Wikimedia Commons NGC 176 on WikiSky: DSS2,...
; Richter, O.-G.; Ferguson, H. C. (February 1992). "H I imaging of NGC3312 and NGC 3314a - A foreground group to the Hydra cluster?". The Astronomical...
3312–3330. arXiv:2108.02791. doi:10.1093/mnras/stab2297. "New General Catalog Objects: NGC 200 - 249". Cseligman. Retrieved September 10, 2016. NGC 220...
NGC 3169 is a spiral galaxy about 75 million light years away in the constellation Sextans. It has the morphological classification SA(s)a pec, which...
NGC 3302 is an unbarred lenticular galaxy in the constellation Antlia. It was discovered by the astronomer John Herschel on January 28, 1835. "NGC 3302"...
NGC 3009 is a lenticular galaxy in the constellation of Ursa Major. It is about 35 thousand light years across, and with a recessional velocity of 4,445...
NGC 3301, also known as NGC 3760, is a lenticular galaxy in the constellation Leo. Its apparent magnitude in the V-band is 11.1. It was first observed...
NGC 3007 is an edge-on, magnitude 13.4, lenticular galaxy in the constellation of Sextans, discovered by Édouard Stephan on March 16, 1855. It is about...
It is a member of the NGC 2998 group, which also includes NGC 2998, NGC 3002, NGC 3006, NGC 3008, and a few others. Skrutskie, Michael F.; Cutri, Roc...
NGC 3486 is an intermediate barred spiral galaxy located about 27.4 million light years away in the constellation of Leo Minor. It has a morphological...
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