17 pages, 9 color figures, uses emulateapj. Version with better resolution figures at http://hea-www.harvard.edu/~maxim/papers/rhalos_tmaps/ . ApJ in pres
We study diffuse radio emission in the galaxy cluster A1550, with the aim of constraining particle r...
International audienceContext. Many galaxy clusters host megaparsec-scale diffuse radio sources call...
We report the detection of a diffuse radio halo source in the hottest known cluster of galaxies 1E06...
A521 is an interacting galaxy cluster located at z = 0.247, hosting a low-frequency radio halo conne...
We report the discovery of spatially-extended, non-thermal-like emission components in Chandra X-ray...
open14siContext. Radio halos and relics are Mpc-scale diffuse radio sources in galaxy clusters, whic...
open7siAcknowledgements. We thank the anonymous referee for the useful comments. The National Radio ...
open11siAcknowledgments The authors thank the anonymous referee for the useful comments which impro...
By analyzing the gas temperature maps created from the Chandra archive data, we reveal the prevailin...
We discuss two themes from Chandra observations of galaxies and clusters. First, we describe the eff...
We present preliminary Chandra results on z=0.2 clusters A665, A2163 and A2218, and a z=0.05 cluster...
Many galaxy clusters host megaparsec-scale radio halos, generated by ultrarelativistic electrons in ...
Context. Many galaxy clusters host megaparsec-scale diffuse radio sources called radio halos. Their ...
Many galaxy clusters host megaparsec-scale radio halos, generated by ultrarelativistic electrons in ...
Extended, steep, and ultra-steep spectrum radio emission in a galaxy cluster is usually associated w...
We study diffuse radio emission in the galaxy cluster A1550, with the aim of constraining particle r...
International audienceContext. Many galaxy clusters host megaparsec-scale diffuse radio sources call...
We report the detection of a diffuse radio halo source in the hottest known cluster of galaxies 1E06...
A521 is an interacting galaxy cluster located at z = 0.247, hosting a low-frequency radio halo conne...
We report the discovery of spatially-extended, non-thermal-like emission components in Chandra X-ray...
open14siContext. Radio halos and relics are Mpc-scale diffuse radio sources in galaxy clusters, whic...
open7siAcknowledgements. We thank the anonymous referee for the useful comments. The National Radio ...
open11siAcknowledgments The authors thank the anonymous referee for the useful comments which impro...
By analyzing the gas temperature maps created from the Chandra archive data, we reveal the prevailin...
We discuss two themes from Chandra observations of galaxies and clusters. First, we describe the eff...
We present preliminary Chandra results on z=0.2 clusters A665, A2163 and A2218, and a z=0.05 cluster...
Many galaxy clusters host megaparsec-scale radio halos, generated by ultrarelativistic electrons in ...
Context. Many galaxy clusters host megaparsec-scale diffuse radio sources called radio halos. Their ...
Many galaxy clusters host megaparsec-scale radio halos, generated by ultrarelativistic electrons in ...
Extended, steep, and ultra-steep spectrum radio emission in a galaxy cluster is usually associated w...
We study diffuse radio emission in the galaxy cluster A1550, with the aim of constraining particle r...
International audienceContext. Many galaxy clusters host megaparsec-scale diffuse radio sources call...
We report the detection of a diffuse radio halo source in the hottest known cluster of galaxies 1E06...
DOI
Add to ORKG