Add to ORKGWe present the latest results from the 150 ks XMM-Newton observation of the most powerful radio halo galaxy cluster MACS J0717.5+3745 (z=0.55). This spectacular merging galaxy cluster reveals important clues into the connection between the population of non-thermal synchrotron emitting particles and the diffuse, X-ray emitting, thermal gas. Utilizing XMM-Newton\u27s excellent collecting area and spatial-resolution, we focus upon the morphology of the thermal properties of the diffuse gas and discuss the presence of a potentially non-thermal X-ray spectral component
International audienceWe present a comprehensive multiwavelength analysis of the merging galaxy clus...
Received; accepted Context. To investigate the non−thermal emission mechanism and their interaction ...
We present an XMM observation of the radio jet and diffuse halo of the nearby radio galaxy NGC6251. ...
Aims. We present the results of a joint XMM-Newton and NuSTAR observation (200 ks) of the galaxy clu...
Open AccessAims. To investigate the nonthermal emission mechanism and their interaction during clust...
International audienceTo investigate the nonthermal emission mechanism and their interaction during ...
Aims. To study at multiple frequencies the radio emission arising from the massive galaxy cluster MA...
Aims. We present the results of a joint XMM-Newton and NuSTAR observation (200 ks) of the galaxy clu...
We present an XMM-Newton observation of the radio jet and diffuse halo of the nearby radio galaxy N...
Context. Mergers of galaxy clusters are among the most energetic events in the Universe. These event...
An XMM-Newton imaging spectroscopy analysis of the galaxy cluster A1644 is presented. A1644 is a com...
Context. Mergers of galaxy clusters are among the most energetic events in the Universe. These event...
Aims. To study at multiple frequencies the radio emission arising from the massive galaxy cluster MA...
We present a deep XMM-Newton observation of the extremely massive, rapidly rotating, relativistic-je...
Aims. To study at multiple frequencies the radio emission arising from the massive galaxy cluster M...
International audienceWe present a comprehensive multiwavelength analysis of the merging galaxy clus...
Received; accepted Context. To investigate the non−thermal emission mechanism and their interaction ...
We present an XMM observation of the radio jet and diffuse halo of the nearby radio galaxy NGC6251. ...
Aims. We present the results of a joint XMM-Newton and NuSTAR observation (200 ks) of the galaxy clu...
Open AccessAims. To investigate the nonthermal emission mechanism and their interaction during clust...
International audienceTo investigate the nonthermal emission mechanism and their interaction during ...
Aims. To study at multiple frequencies the radio emission arising from the massive galaxy cluster MA...
Aims. We present the results of a joint XMM-Newton and NuSTAR observation (200 ks) of the galaxy clu...
We present an XMM-Newton observation of the radio jet and diffuse halo of the nearby radio galaxy N...
Context. Mergers of galaxy clusters are among the most energetic events in the Universe. These event...
An XMM-Newton imaging spectroscopy analysis of the galaxy cluster A1644 is presented. A1644 is a com...
Context. Mergers of galaxy clusters are among the most energetic events in the Universe. These event...
Aims. To study at multiple frequencies the radio emission arising from the massive galaxy cluster MA...
We present a deep XMM-Newton observation of the extremely massive, rapidly rotating, relativistic-je...
Aims. To study at multiple frequencies the radio emission arising from the massive galaxy cluster M...
International audienceWe present a comprehensive multiwavelength analysis of the merging galaxy clus...
Received; accepted Context. To investigate the non−thermal emission mechanism and their interaction ...
We present an XMM observation of the radio jet and diffuse halo of the nearby radio galaxy NGC6251. ...