Galaxy in the constellation Leo
NGC 3883 is a large[ 3] low surface brightness [ 4] [ 5] spiral galaxy located about 330 million light-years away[ 6] in the constellation Leo .[ 7] NGC 3883 has a prominent bulge but does not host an AGN . The galaxy also has flocculent spiral arms in its disk.[ 5] It was discovered by astronomer William Herschel on April 13, 1785[ 8] and is a member of the Leo Cluster .[ 3] [ 9]
^ a b c d e f g h i "NASA/IPAC Extragalactic Database" . Results for NGC 3883 . Retrieved 2018-08-04 .
^ Schombert, J. (1998). "Active Galactic Nucleus Activity in Giant, Low Surface Brightness Galaxies" . The Astronomical Journal . 116 (4): 1650–1656. Bibcode :1998AJ....116.1650S . doi :10.1086/300558 . ISSN 1538-3881 .
^ a b M., van der Hulst, J.; D., Skillman, E.; C., Kennicutt, R.; D., Bothun, G. (May 1987). "The neutral hydrogen content of red spiral galaxies". Astronomy and Astrophysics . 177 : 63. Bibcode :1987A&A...177...63V . ISSN 0004-6361 . {{cite journal }}
: CS1 maint: multiple names: authors list (link )
^ Impey, Chris; Bothun, Greg (June 1, 1989). "Malin 1 - A quiescent disk galaxy" . The Astrophysical Journal . 341 : 89–104. Bibcode :1989ApJ...341...89I . doi :10.1086/167474 . ISSN 0004-637X .
^ a b Ramya, S.; Prabhu, T. P.; Das, M. (2011-12-01). "Active galactic nucleus activity and black hole masses in low surface brightness galaxies" . Monthly Notices of the Royal Astronomical Society . 418 (2): 789–800. arXiv :1108.0763 . Bibcode :2011MNRAS.418..789R . doi :10.1111/j.1365-2966.2011.19530.x . ISSN 0035-8711 . S2CID 119279755 .
^ "Your NED Search Results" . ned.ipac.caltech.edu . Retrieved 2018-08-05 .
^ "Revised NGC Data for NGC 3883" . spider.seds.org . Retrieved 2018-08-05 .
^ "New General Catalog Objects: NGC 3850 - 3899" . cseligman.com . Retrieved 2018-07-17 .
^ "NGC 3883" . Retrieved 2018-08-06 .