| 词条 | NGC 1409 |
| 释义 |
NGC 1409 is an interacting elliptical galaxy in the constellation Taurus. There appears to be a pipeline of gas being funneled from NGC 1409 to NGC 1410. This pipeline is creating significant stellar birth in NGC 1410. {{Infobox Galaxy| name = NGC 1409 | image = NGC 1409HSTFull.jpg | image_size = 250px | caption = A Hubble Space Telescope (HST) image of NGC 1410 (left) and NGC 1409 (right) | credit= HST/NASA/ESA | constellation name = Taurus[1] | epoch = J2000 | type = SAB pec[2] | ra = {{RA|3|41|10.4}}[2] | dec = {{DEC|-1|18|9}}[2] | dist_ly = | z = 7750 ± 40 km/s[2] | appmag_v = 15.4[2] | size_v = 1′.0 × 0′.8[2] | notes = | names = UGC 2821,[2] PGC 13553[2] }} See also
External links
References1. ^{{cite web | title=HubbleSite - NewsCenter - Intergalactic 'Pipeline' Funnels Matter Between Colliding Galaxies | url=http://hubblesite.org/newscenter/archive/releases/2001/02/fastfacts/ | accessdate=2007-04-05}} {{Ngc15}}{{galaxy-stub}}2. ^1 2 3 4 5 6 7 {{cite web | title=NASA/IPAC Extragalactic Database | work=Results for NGC 1409 | url=http://nedwww.ipac.caltech.edu/ | accessdate=2007-04-05}} 6 : Interacting galaxies|Intermediate spiral galaxies|Taurus (constellation)|NGC objects|UGC objects|Principal Galaxies Catalogue objects |
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