ESO 501-38, AM 1034-271, MCG -4-25-36, PGC 31478[1]
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NGC 3311 is a super-giant[2] elliptical galaxy[3] (a type-cD galaxy)[4][3] located about 190 million light-years away[5] in the constellation Hydra.[6] The galaxy was discovered by astronomer John Herschel on March 30, 1835.[7][8] NGC 3311 is the brightest[9][10] member of the Hydra Cluster[11] and forms a pair with NGC 3309 which along with NGC 3311, dominate the central region of the Hydra Cluster.[12]
NGC 3311 is surrounded by a rich and extensive globular cluster system[13] rivaling that of Messier 87 in the Virgo Cluster.[4]
^ abcdefghij"NASA/IPAC Extragalactic Database". Results for NGC 3311. Retrieved 2018-05-22.
^ abBely, Pierre-Yves; Christian, Carol; Roy, Jean-René (2010-03-11). A Question and Answer Guide to Astronomy. Cambridge University Press. ISBN 978-0-521-18066-5.
^ abCite error: The named reference :0 was invoked but never defined (see the help page).
^"Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-05-24.
^"Revised NGC Data for NGC 3311". spider.seds.org. Retrieved 2018-05-24.
^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.
^Barbosa, C. E.; Arnaboldi, M.; Coccato, L.; Gerhard, O.; Mendes de Oliveira, C.; Hilker, M.; Richtler, T. (January 2018). "Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I cluster". Astronomy & Astrophysics. 609: A78. arXiv:1710.08941. Bibcode:2018A&A...609A..78B. doi:10.1051/0004-6361/201731834. ISSN 0004-6361. S2CID 73534240.
^"NGC 3311". Retrieved 2018-05-26.
^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.
^Kotanyi, C. (November 1990). "NGC 3309: an S-shaped radio galaxy in a nearby cluster". Revista Mexicana de Astronomía y Astrofísica. 21: 173–176. Bibcode:1990RMxAA..21..173K.
^Cite error: The named reference :4 was invoked but never defined (see the help page).
NGC3311 is a super-giant elliptical galaxy (a type-cD galaxy) located about 190 million light-years away in the constellation Hydra. The galaxy was discovered...
cluster's largest galaxies are elliptical galaxies NGC 3309 and NGC3311 and the spiral galaxy NGC 3312 all having a diameter of about 150,000 light-years...
galaxy forms a pair with NGC3311 which lies about 72,000 ly (22 kpc) away. Both galaxies dominate the center of the Hydra Cluster. NGC 3309 has a radio jet...
supermassive black hole. NGC 154, a similar elliptical galaxy NGC 3640, a similar elliptical galaxy with around the same size. NGC3311, a supergiant elliptical...
Other galaxies with rich globular cluster systems are NGC 4874, NGC 4889, NGC3311 and Messier 87. For comparison, the Milky Way has a poor globular cluster...
NGC 3312 was distorted by the giant elliptical galaxies NGC 3309 and NGC3311 which are the dominant ellipticals in the Hydra Cluster. However, NGC 3309...
include NGC 3805, NGC 3837, the brightest cluster member NGC 3842, NGC 3860, NGC 3883, NGC 3884, NGC 3919, NGC 3929, NGC 3937, NGC 3940 and NGC 3954. Other...
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 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 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 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...
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...
83. Positioned just 1.8° to the south-southwest is the planetary nebula NGC 3242. Mu Hydrae has an annual parallax shift of 13.93 mas, which yields a...
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...
light-years from the Sun. It is a member of the NGC 2998 group, which also includes NGC 2998, NGC 3002, NGC 3005, NGC 3006, and a few others. Among these galaxies...