| 词条 | NGC 4262 |
| 释义 |
| name = NGC 4262 | image = NGC_4262_HST_9401_R850GB475.png | caption = Composite image of NGC 4262, imaged by the Hubble Space Telescope | epoch = J2000 | type = SB(s)0−[1] | ra = {{RA|12|19|30.6}}[1] | dec = {{DEC|+14|52|40}}[1] | dist_ly = 50.0 Mly | z = 1359 ± 4 km/s[1] | appmag_v = 12.49[1] | size_v = 1′.9 × 1′.7[1] | constellation name = Coma Berenices | names = UGC 7365,[1] PGC 39676, VCC 355[1] }} NGC 4262 is a galaxy located in the constellation of Coma Berenices. CharacteristicsNGC 4262 is a small and compact barred lenticular galaxy with a high surface brightness central bar.[2] It is a member of the Virgo Cluster at a distance from the Milky Way of around 50 million light-years.[3] It features an anomalous abundance of neutral hydrogen for a lenticular galaxy, most of it being located on a ring tilted with respect to NGC 4262's galactic plane.[4] Studies with help of the GALEX telescope have found within that ring several clusters of young stars that can be seen on ultraviolet images.[5] The aforementioned ring is believed to have its origin in NGC 4262 stripping some gas of another galaxy in a close passage, likely its neighbor the spiral Messier 99[6] References1. ^1 2 3 4 5 6 7 {{cite web | title=NASA/IPAC Extragalactic Database | work=Results for NGC 4262 | url=http://nedwww.ipac.caltech.edu/ | accessdate=2012-12-31}} {{Ngc45}}2. ^{{cite web |title=Notes for object NGC 4262 |publisher=NASA/IPAC Extragalactic Database (NED) |url=http://ned.ipac.caltech.edu/cgi-bin/nph-datasearch?search_type=Note_id&objid=29953&objname=NGC%204262&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table |accessdate=2012-07-21}} 3. ^{{Cite journal | last1 = Mei | first1 = S. | last2 = Blakeslee | first2 = J. P. | last3 = Côté | first3 = P. | last4 = Tonry | first4 = J.L. | last5 = West | first5 = M. J. | last6 = Ferrarese. | first6 = L. | last7 = Jordán | first7 = A. | last8 = Peng | first8 = E. W. | last9 = Anthony | first9 = A. | last10 = Merritt | first10 = D. | date = January 2007 | journal = The Astrophysical Journal | volume = 655 | issue = 1 | pages = 144–162 | title = The ACS Virgo Cluster Survey. XIII. SBF Distance Catalog and the Three-dimensional Structure of the Virgo Cluster |arxiv = astro-ph/0702510 |bibcode = 2007ApJ...655..144M |doi = 10.1086/509598 }} 4. ^{{Cite journal | last1 = Krumm | first1 = N. | last2 = van Driel | first2 = W. | last3 = van Woerden | first3 = H. | date = March 1985 | journal = Astronomy and Astrophysics | volume = 144 | issue = 1 | pages = 202–210 | title = Distribution and motions of atomic hydrogen in lenticular galaxies. IV - A ring of H I around NGC 4262 |bibcode = 1985A&A...144..202K }} 5. ^{{Cite journal | last1 = Bettoni | first1 = D. | last2 = Buson | first2 = L.M. | last3 = Galletta | first3 = G. | date = September 2010 | doi = 10.1051/0004-6361/201014750 | journal = Astronomy and Astrophysics | volume = 519 | issue = A72 | pages = A72 | title = NGC 4262: a Virgo galaxy with an extended ultraviolet ring | bibcode = 2010A&A...519A..72B| arxiv = 1006.4717 }} 6. ^{{Cite journal | last1 = Vollmer | first1 = B. | last2 = Hutchmeier | first2 = W. | last3 = van Driel | first3 = W. | date = September 2005 | journal = Astronomy and Astrophysics | volume = 439 | issue = 3 | pages = 921–933 | title = NGC 4254: a spiral galaxy entering the Virgo cluster |arxiv = astro-ph/0505021 |bibcode = 2005A&A...439..921V |doi = 10.1051/0004-6361:20041350 }} 5 : Lenticular galaxies|Barred lenticular galaxies|Virgo Cluster|Coma Berenices (constellation)|NGC objects |
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