2001:B011:B807:D419:D543:28E8:A34D:C321：/* top */ 修正筆誤

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{{noteTA
|G1 = Astronomy
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[[File:Color image of galaxy cluster MCS J0416.1–2403.jpg|thumb|[[哈勃空间望远镜]]拍攝的星系團MCS J0416.1–2403。]]

'''MACS J0416.1-2403'''是一個[[紅移]]值 z=0.397 的星系團，位於[[波江座]]<ref>{{cite web |url=https://www.spacetelescope.org/images/heic1416a/ |title=Colour image of galaxy cluster MCS J0416.1–2403 |last= |first= |date=24 July 2014 |publisher=ESA/Hubble |accessdate=6 September 2015 |archive-date=2020-10-25 |archive-url=https://web.archive.org/web/20201025052556/https://www.spacetelescope.org/images/heic1416a/ |dead-url=no }}</ref>。200 [[秒差距|kpc]]範圍內質量為太陽的160兆倍。如果它的半徑是950 kpc，總質量則是太陽的1.15 x 10<sup>15</sup>倍<ref name="Jauzac">{{cite web |url=http://arxiv.org/abs/1406.3011 |title=Hubble Frontier Fields: The Geometry and Dynamics of the Massive Galaxy Cluster Merger MACSJ0416.1-2403 |last=Jauzac |first=Mathilde |author2=Eric Jullo |author3=Dominique Eckert |author4=Harald Ebeling |author5=Johan Richard |author6=Marceau Limousin |display-authors=etal |date=23 June 2014 |publisher=arXiv |accessdate=25 July 2014 |archive-date=2019-09-30 |archive-url=https://web.archive.org/web/20190930153834/https://arxiv.org/abs/1406.3011 |dead-url=no }}</ref>。該星系團由{{link-en|大質量星系團巡天|MAssive Cluster Survey}}發現（Massive Cluster Survey, MACS）<ref name="Mann & Ebeling">{{cite web |url=http://adsabs.harvard.edu/abs/2012MNRAS.420.2120M |title=X-ray-optical classification of cluster mergers and the evolution of the cluster merger fraction |last=Mann |first=Andrew |author2=Harald Ebeling |date=March 2012 |accessdate=2015-09-06 |archive-date=2018-08-08 |archive-url=https://web.archive.org/web/20180808123924/http://adsabs.harvard.edu/abs/2012MNRAS.420.2120M |dead-url=no }}</ref><ref name="MACS">{{cite web |url=http://adsabs.harvard.edu/abs/2001ApJ...553..668E |title=MACS: A Quest for the Most Massive Galaxy Clusters in the Universe |last=Ebeling |first=Harald |author2=Alastair Edge |author3=J. Patrick Henry |date=June 2001 |accessdate=3 February 2015 |archive-date=2019-03-30 |archive-url=https://web.archive.org/web/20190330151909/http://adsabs.harvard.edu/abs/2001ApJ...553..668E |dead-url=no }}</ref>。該星系團可使位於它後方遠處的星系產生[[重力透鏡]]效應，使一個星系產生多個影像<ref>{{cite web |url=http://adsabs.harvard.edu/abs/2014arXiv1406.1217D |title=Free Form Lensing Implications for the Collision of Dark Matter and Gas in the Frontier Fields Cluster MACSJ0416.1-2403 |last=Diego |first=Jose M. |date=4 June 2014 |accessdate=2015-09-06 |archive-date=2018-08-08 |archive-url=https://web.archive.org/web/20180808112756/http://adsabs.harvard.edu/abs/2014arXiv1406.1217D |dead-url=no }}</ref><ref>{{cite web |url=http://phys.org/news/2014-07-mass-distant-galaxy-cluster-precise.html |title=New mass map of a distant galaxy cluster is the most precise yet |date=24 July 2014 |accessdate=25 July 2014 |archive-date=2019-08-24 |archive-url=https://web.archive.org/web/20190824061843/https://phys.org/news/2014-07-mass-distant-galaxy-cluster-precise.html |dead-url=no }}</ref>。

==參考資料==
{{Reflist}}

[[Category:星系團]]
[[Category:波江座]]

MACS0416.1-2403 - 版本历史

2001:B011:B807:D419:D543:28E8:A34D:C321：​/* top */ 修正筆誤

2001:B011:B807:D419:D543:28E8:A34D:C321：/* top */ 修正筆誤