Spiral galaxy in the constellation Dorado
NGC 1892 is aspiral galaxy located approximately 51 millionlight-years away[ 5] Dorado . It was discovered November 30, 1834 byJohn Herschel .[ 3] NGC 1947 Group [ 6] [ 7] [ 8] Southern Supercluster .[ 7]
NGC 1892, despite being a spiral galaxy, has a centralbulge which is morphologically more similar todwarf irregular galaxies . The galaxy's central bulge which is highly irregular, is obscured by a dust lane.[ 9] nuclear star cluster [ 10] 6 M ☉ [ 11] supermassive black hole with an estimated mass 4.7 × 106 M ☉ [ 12]
A probablesupernova of typeIIP was photographed by theCarnegie-Irvine Galaxy Survey (CGS) in 2004,[ 13] [ 5]
^a b c d e f g "NED results for object NGC 1892" .NASA/IPAC EXTRAGALACTIC DATABASE . Caltech. Retrieved29 September 2018 .^a b c d Guillochon, James; Stockler de Moraes, Jorge; Nicholl, Matt; Patnaude, Daniel J; Auchetti, Katie; Barth, Aaron J; Ho, Luis C; Li, Zhao-Yu; Carnegie-Irvine Galaxy Survey (2018)."Serendipitous Discovery of a 14 year old Supernova at 16 Mpc" .Research Notes of the AAS .2 (3): 165.arXiv :1809.00163 Bibcode :2018RNAAS...2..165G .doi :10.3847/2515-5172/aade89 S2CID 119431988 . ^a b c Seligman, Courtney."Celestial Atlas NGC Objects 1850-1899" .cseligman.com . Retrieved29 September 2018 . ^ "NGC 1892" .SIMBAD . Retrieved29 September 2018 .^a b Kohler, Susanna (2018)."Surprise Discovery of a 14-Year-Old Supernova" .Aas Nova Highlights : 4028.Bibcode :2018nova.pres.4028K . Retrieved29 September 2018 . ^ Tully, R. Brent (1988).Nearby galaxies catalog (1. publ ed.). Cambridge: Cambridge University Press.ISBN 978-0-521-35299-4 ^a b Fouque, P.; Gourgoulhon, E.; Chamaraux, P.; Paturel, G. (1992-05-01)."Groups of galaxies within 80 Mpc. II. The catalogue of groups and group members" .Astronomy and Astrophysics Supplement Series .93 :211– 233.Bibcode :1992A&AS...93..211F .ISSN 0365-0138 . ^ Giuricin, Giuliano; Marinoni, Christian; Ceriani, Lorenzo; Pisani, Armando (2000-11-01)."Nearby Optical Galaxies: Selection of the Sample and Identification of Groups" .The Astrophysical Journal .543 (1):178– 194.arXiv :astro-ph/0001140 Bibcode :2000ApJ...543..178G .doi :10.1086/317070 .ISSN 0004-637X . ^ Carollo, C. M.; Stiavelli, M.; de Zeeuw, P. T.; Mack, J. (1997-12-01)."Spiral Galaxies with WFPC2.I.Nuclear Morphology, Bulges, Star Clusters, and Surface Brightness Profiles" .The Astronomical Journal .114 : 2366.Bibcode :1997AJ....114.2366C .doi :10.1086/118654 .ISSN 0004-6256 . ^ Georgiev, Iskren Y.; Böker, Torsten (2014-07-11)."Nuclear star clusters in 228 spiral galaxies in the HST/WFPC2 archive: catalogue and comparison to other stellar systems" .Monthly Notices of the Royal Astronomical Society .441 (4):3570– 3590.arXiv :1404.5956 doi :10.1093/mnras/stu797 ISSN 1365-2966 . ^ Georgiev, Iskren Y.; Böker, Torsten; Leigh, Nathan; Lützgendorf, Nora; Neumayer, Nadine (2016-04-01)."Masses and scaling relations for nuclear star clusters, and their co-existence with central black holes" .Monthly Notices of the Royal Astronomical Society .457 (2):2122– 2138.arXiv :1601.02613 Bibcode :2016MNRAS.457.2122G .doi :10.1093/mnras/stw093 ISSN 0035-8711 . ^ Arzoumanian, Zaven; Baker, Paul T.; Brazier, Adam; Brook, Paul R.; Burke-Spolaor, Sarah; Becsy, Bence; Charisi, Maria; Chatterjee, Shami; Cordes, James M.; Cornish, Neil J.; Crawford, Fronefield; Cromartie, H. Thankful; Decesar, Megan E.; Demorest, Paul B.; Dolch, Timothy (2021-06-01)."The NANOGrav 11 yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500 Mpc" .The Astrophysical Journal .914 (2): 121.arXiv :2101.02716 Bibcode :2021ApJ...914..121A .doi :10.3847/1538-4357/abfcd3 ISSN 0004-637X . ^ "NGC 1892" .The Carnegie-Irvine Galaxy Survey (CGS) . Retrieved29 September 2018 .NGC 1892 at Wikimedia Commons
Media related toNGC 1892 at Wikimedia Commons