The Hubble Space Telescope Frontier Fields cluster MACS J1149.6+2223 is one of the most complex merging clusters, believed to consist of four dark matter halos. We present results from deep (365 ks) Chandra observations of the cluster, which reveal the most distant cold front (z = 0.544) discovered to date. In the cluster outskirts, we also detect hints of a surface brightness edge that could be the bow shock preceding the cold front. The substructure analysis of the cluster identified several components with large relative radial velocities, thus indicating that at least some collisions occur almost along the line of sight. The inclination of the mergers with respect to the plane of the sky poses significant observational challenges at X...
[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway...
open14siContext. Radio halos and relics are Mpc-scale diffuse radio sources in galaxy clusters, whic...
© 2016 The Authors. We present a 66 ks Chandra X-ray observation of the galaxy cluster RXJ0334.2-011...
The Hubble Space Telescope Frontier Fields cluster MACS J1149.6+2223 is one of the most complex merg...
The Hubble Space Telescope Frontier Fields cluster MACS J1149.6+2223 is one of the most complex merg...
Merging galaxy clusters leave long-lasting signatures on the baryonic and non-baryonic cluster const...
Merging galaxy clusters leave long-lasting signatures on the baryonic and non-baryonic cluster const...
Merging galaxy clusters leave long-lasting signatures on the baryonic and non-baryonic cluster const...
International audienceWe use a joint optical/X-ray analysis to constrain the geometry and history of...
International audienceWe use a joint optical/X-ray analysis to constrain the geometry and history of...
We use a joint optical/X-ray analysis to constrain the geometry and history of the ongoing merging e...
To investigate the relationship between thermal and non-thermal components in merger galaxy clusters...
[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway...
open14siContext. Radio halos and relics are Mpc-scale diffuse radio sources in galaxy clusters, whic...
© 2016 The Authors. We present a 66 ks Chandra X-ray observation of the galaxy cluster RXJ0334.2-011...
The Hubble Space Telescope Frontier Fields cluster MACS J1149.6+2223 is one of the most complex merg...
The Hubble Space Telescope Frontier Fields cluster MACS J1149.6+2223 is one of the most complex merg...
Merging galaxy clusters leave long-lasting signatures on the baryonic and non-baryonic cluster const...
Merging galaxy clusters leave long-lasting signatures on the baryonic and non-baryonic cluster const...
Merging galaxy clusters leave long-lasting signatures on the baryonic and non-baryonic cluster const...
International audienceWe use a joint optical/X-ray analysis to constrain the geometry and history of...
International audienceWe use a joint optical/X-ray analysis to constrain the geometry and history of...
We use a joint optical/X-ray analysis to constrain the geometry and history of the ongoing merging e...
To investigate the relationship between thermal and non-thermal components in merger galaxy clusters...
[[sponsorship]]天文及天文物理研究所[[note]]已出版;[SCI];有審查制度;具代表性[[note]]http://gateway.isiknowledge.com/gateway...
open14siContext. Radio halos and relics are Mpc-scale diffuse radio sources in galaxy clusters, whic...
© 2016 The Authors. We present a 66 ks Chandra X-ray observation of the galaxy cluster RXJ0334.2-011...