sponsored by psychohistorian.org
Type: galaxy (Seyfert 1), Sb
Mag: B=13.52, V=?
Size: 6.165′ x 4.466′
PA: 155°
Synonyms: H II-029
One of a close pair of galaxies due East of Gamma Leonis, the other being NGC 3226. Discovered in 1784 by William Herschel with an 18.7-inch f/13 speculum telescope. He called it "Two, about 2' asunder. Both faint, considerably large, round."
A supernova erupted in this galaxy in 1983 (12.0v)
Together with NGC 3226 listed as No. 94 in Arp's "Atlas of Peculiar Galaxies" (Astrophysical Journal Supplement, vol. 14, 1966.) He remarks "companion on edge of large, very faint loop extending opposite galaxy."
The RNGC (Sulentic and Tifft 1973) notes that this is a 12.0 mag galaxy. Their coded description reads EL,BCTW/DKLNS VFDIFO ARMS.
G. de Vaucouleurs ("Galaxies and the Universe", Chapter 14 - Nearby Groups of Galaxies) notes that the NGC 3190 Group is a part of the Leo II Cloud Complex. The five brightest members of the NGC 3190 Group are NGC 3227, NGC 3190, NGC 3162, NGC 3193 & NGC 3226.
Van den Bergh (1961, Astronomical Journal, Vol 66, p566) notes that this galaxy forms a pure pair with NGC 3226 2.3 arcminutes away.
This galaxy is listed in the "Third Reference Catalogue of Bright Galaxies" as being a bright Seyfert galaxy. The integrated B magnitude of the stellar system (excluding the nucleus) = 11.58, and the B magnitude of the quasi-stellar nucleus = 15.00.
Photo Index by Jim Lucyk: The Astrograph 6-7/88 p89, Observer's Guide (Astro Cards) 3-4/88 p21.
Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: "11.6M; 3' x 1.2' extent; soft, centerless oblong; EL GAL N3226 (H29-1)(12.7M; 1' diameter) 2' to NNW; soft and round; !good supernova prospects! just W of Algieba (Gamma LEO)."
Observing site: Pinnacles overlook
Telescope: C-8
[10h 23m 30s, 19° 52m 0s] The expected bright nucleus of this Seyfert was quite faint.
Lacaille's catalogue
The Messier objects
Dunlop's catalogue
The Bennett objects
The Caldwell list
Named DSOs
DOCdb is still in beta-release.
Known issues, feature requests, and updates on bug fixes, are here:
Found a bug? Have a comment or suggestion to improve DOCdb? Please let us know!
DOCdb is a free online resource that exists to promote deep sky observing.
You could help by sharing your observations, writing an article, digitizing and proof-reading historical material, and more.
Everything on DOCdb.net is © 2004-2010 by Auke Slotegraaf, unless stated otherwise or if you can prove you have divine permission to use it. Before using material published here, please consult the Creative Commons Attribution-Non-Commercial-Share Alike 2.5 License. Some material on DOCdb is copyright the individual authors. If in doubt, don't reproduce. And that goes for having children, too. Please note that the recommended browser for DOCdb is Firefox 3.x. You may also get good results with K-Meleon. Good luck if you're using IE. A successful experience with other browsers, including Opera and Safari, may vary.