Description | Images |
Object name: NGC6240Designation(s): NGC6240, How Arp missed or decided against putting this rather famous galaxy in his catalog I can't fathom. During the time of his atlas, the best anyone could do in understanding this one was shown in comments like this from a 1964 paper: "Complex core with strong dark lane. Distorted. Faint outer filament. No nearby object of similar size. Another very peculiar object." We now know this is the result of a galaxy merger. It has two nuclei only 1.8" apart. As the early paper says it is quite alone in space. This makes the merger all the more surprising. The galaxy is a super-luminous IRAS (infrared) galaxy and a starburst galaxy. Both likely the result of the merger. It has spectral characteristics of LINER and Seyfert 2 galaxies. Redshift puts it 335 million light-years away and is seen against the stars of Ophiuchus. It is well covered by the HST. They say it is 400 million light-years distant. I can't explain the difference but it does show the difficulty of determining distance to such objects. It was discovered by Édouard Stephan on July 12, 1871. For further information on this merger and to see the great HST image of it go to: http://www.spacetelescope.org/static/archives/images/large/heic0810ai.jpg Related Designation(s):1RXP J165259.0+022406, 1RXS J165257.9+022353, 2MASX J16525886+0224035, 2PBC J1653.0+0223, 2XMM J165258.9+022403, 2XMMp J165258.9+022403, 4C +02.44, 87GB 165028.6+022854, 87GB[BWE91] 1650+0228, AKARI J1652589+022408, C-GOALS 30, CGCG 025-011, CGCG 1650.5+0229, CXO J165258.8+022403, IC 4625, IRAS 16504+0228, IRAS F16504+0228, MCG +00-43-004, MG1 J165303+0222, MRC 1650+024, NGC 6240, NGC 6240:[HAS2013] N, NGC 6240:[HAS2013] S, NGC6240, NSA 147462, NVSS J165258+022403, PGC 059186, PKS 1650+024, PKS B1650+024, PKS J1652+0224, PMN J1653+0224, PRC D-28, RGB J1652+024, RX J1652.9+0223, SDSS J165258.89+022402.8, SWIFT J1652.9+0223, SWIFT J1653.2+0224, TXS 1650+024, UGC 10592, UZC J165259.0+022407, VV 617, [AHG2014] B214, [dML87] 701, [FBS2007] 53, [GMM2009b] 74, [KRL2007] 206, [VCV2001] J165258.9+022401, [VCV2006] J165258.9+022401, [WB92] 1650+0228, [WMR2009] 120, |