We report the discovery of the merging cluster, RXCJ2359.3-6042, from the REFLEX II cluster survey and present our results from all three detectors combined in the imaging and spectral analysis of the XMM-Newton data. Also known as Abell 4067, this is a unique system, where a compact bullet penetrates an extended, low density cluster at redshift z = 0.0992 clearly seen from our follow-up XMM-Newton observation. The bullet goes right through the central region of the cluster without being disrupted and we can clearly see how the bullet component is stripped of its layers outside the core. There is an indication of a shock heated region in the east of the cluster with a higher temperature. The bulk temperature of the cluster is about 3.12(±0....
Abell 1758 was classified as a single rich cluster of galaxies by Abell, but a ROSAT observation sho...
© 2021. The American Astronomical Society. We present high-resolution optical images from the Hubble...
Using a combination of Chandra and XMM observations, we confirmed the presence of a significant velo...
Abell 3266 is one of the X-ray brightest galaxy clusters in the sky and is a well-known merging syst...
(Abridged) The galaxy cluster Abell 2218, at z=0.171, is well-known for the discrepancy between mass...
We present the results of deep 140 ks Suzaku X-ray observations of the north-east (NE) radio relic o...
We present the results of a detailed analysis of the XMM-Newton observation of the galaxy cluster A...
We present an X-ray spectral analysis using XMM-Newton/EPIC observations (∼100 ks) of the merging ga...
Mergers between galaxy clusters are an important stage in the formation of the large-scale structure...
Galaxy cluster mergers are excellent laboratories for studying numerous physical processes. Differen...
An XMM-Newton imaging spectroscopy analysis of the galaxy cluster A1644 is presented. A1644 is a com...
We present the results of deep Chandra and XMM-Newton observations of a complex merging galaxy clust...
none8siRadio relics at the peripheries of galaxy clusters are tracers of the elusive cluster merger ...
Abstract. The Bullet Cluster (1E0657-56) merger is of exceptional interest for testing the standard ...
Located at z = 0.203, A2163 is a rich galaxy cluster with an intra-cluster medium (ICM) th...
Abell 1758 was classified as a single rich cluster of galaxies by Abell, but a ROSAT observation sho...
© 2021. The American Astronomical Society. We present high-resolution optical images from the Hubble...
Using a combination of Chandra and XMM observations, we confirmed the presence of a significant velo...
Abell 3266 is one of the X-ray brightest galaxy clusters in the sky and is a well-known merging syst...
(Abridged) The galaxy cluster Abell 2218, at z=0.171, is well-known for the discrepancy between mass...
We present the results of deep 140 ks Suzaku X-ray observations of the north-east (NE) radio relic o...
We present the results of a detailed analysis of the XMM-Newton observation of the galaxy cluster A...
We present an X-ray spectral analysis using XMM-Newton/EPIC observations (∼100 ks) of the merging ga...
Mergers between galaxy clusters are an important stage in the formation of the large-scale structure...
Galaxy cluster mergers are excellent laboratories for studying numerous physical processes. Differen...
An XMM-Newton imaging spectroscopy analysis of the galaxy cluster A1644 is presented. A1644 is a com...
We present the results of deep Chandra and XMM-Newton observations of a complex merging galaxy clust...
none8siRadio relics at the peripheries of galaxy clusters are tracers of the elusive cluster merger ...
Abstract. The Bullet Cluster (1E0657-56) merger is of exceptional interest for testing the standard ...
Located at z = 0.203, A2163 is a rich galaxy cluster with an intra-cluster medium (ICM) th...
Abell 1758 was classified as a single rich cluster of galaxies by Abell, but a ROSAT observation sho...
© 2021. The American Astronomical Society. We present high-resolution optical images from the Hubble...
Using a combination of Chandra and XMM observations, we confirmed the presence of a significant velo...