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后发座纤维状结构

维基百科,自由的百科全书

后发座纤维状结构是一个大尺度纤维状结构.[1][2]这个纤维状结构包含后发座超星系团 ,形成CfA2长城的一部分。[3][4]

参见

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引用

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  1. ^ Finoguenov, A.; Briel, U. G.; Henry, J. P. XMM-Newton Discovery of an X-Ray Filament in Coma. Astrophysics and Space Science Library (Springer Science & Business Media). 2013, 309: 45 [30 May 2017]. ISBN 9781402025648 (英语). 
  2. ^ Fontanelli, P. The Coma/A 1367 filament of galaxies. Astronomy and Astrophysics. September 1984, 138 (1): 85–92. Bibcode:1984A&A...138...85F. ISSN 0004-6361. 
  3. ^ THE ASTRONOMICAL JOURNAL, 115:1745-1777, 1998 May ; THE STAR FORMATION PROPERTIES OF DISK GALAXIES: Hα IMAGING OF GALAXIES IN THE COMA SUPERCLUSTER
  4. ^ Fuller, C.; Davies, J. I.; Smith, M. W. L. H-ATLAS: The Far-Infrared properties of galaxies in and around the Coma Cluster. Monthly Notices of the Royal Astronomical Society. 9 March 2016, 458: 582. Bibcode:2016MNRAS.458..582F. arXiv:1603.02970可免费查阅. doi:10.1093/mnras/stw305.