MACS0416.1-2403
MACS J0416.1-2403是一个红移值 z=0.397 的星系团，位于波江座[1]。200 kpc范围内质量为太阳的160兆倍。如果它的半径是950 kpc，总质量则是太阳的1.15 x 1015倍[2]。该星系团由大质量星系团巡天发现（Massive Cluster Survey, MACS）[3][4]。该星系团可使位于它后方远处的星系产生重力透镜效应，使一个星系产生多个影像[5][6]。
参考资料
[编辑]- ^ Colour image of galaxy cluster MCS J0416.1–2403. ESA/Hubble. 24 July 2014 [6 September 2015]. （原始内容存档于2020-10-25）.
- ^ Jauzac, Mathilde; Eric Jullo; Dominique Eckert; Harald Ebeling; Johan Richard; Marceau Limousin; et al. Hubble Frontier Fields: The Geometry and Dynamics of the Massive Galaxy Cluster Merger MACSJ0416.1-2403. arXiv. 23 June 2014 [25 July 2014]. （原始内容存档于2019-09-30）.
- ^ Mann, Andrew; Harald Ebeling. X-ray-optical classification of cluster mergers and the evolution of the cluster merger fraction. March 2012 [2015-09-06]. （原始内容存档于2018-08-08）.
- ^ Ebeling, Harald; Alastair Edge; J. Patrick Henry. MACS: A Quest for the Most Massive Galaxy Clusters in the Universe. June 2001 [3 February 2015]. （原始内容存档于2019-03-30）.
- ^ Diego, Jose M. Free Form Lensing Implications for the Collision of Dark Matter and Gas in the Frontier Fields Cluster MACSJ0416.1-2403. 4 June 2014 [2015-09-06]. （原始内容存档于2018-08-08）.
- ^ New mass map of a distant galaxy cluster is the most precise yet. 24 July 2014 [25 July 2014]. （原始内容存档于2019-08-24）.