An X-ray/optical study of the geometry and dynamics of MACS J0140.0−0555, a massive post-collision cluster merger

Author:

Ho I-Ting1,Ebeling Harald1,Richard Johan2

Affiliation:

1. Institute for Astronomy; University of Hawaii; 2680 Woodlawn Drive; Honolulu; HI; 96822; USA

2. Centre de Recherche Astrophysique de Lyon; Université Lyon 1; 9 Avenue Charles André; 69561; Saint Genis Laval Cedex; France

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Science from a glimpse: Hubble SNAPshot observations of massive galaxy clusters;Monthly Notices of the Royal Astronomical Society;2018-06-08

2. What if LIGO’s gravitational wave detections are strongly lensed by massive galaxy clusters?;Monthly Notices of the Royal Astronomical Society;2018-01-11

3. Fully stripped? The dynamics of dark and luminous matter in the massive cluster collision MACSJ0553.4−3342;Monthly Notices of the Royal Astronomical Society;2017-06-29

4. The three-dimensional geometry and merger history of the massive galaxy cluster MACS J0358.8−2955;Monthly Notices of the Royal Astronomical Society;2012-12-06

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