XMM-Newton AO-1 observations three SHARC galaxy clusters
| dc.creator | Majerowicz, Sebastien | |
| dc.creator | Arnaud, Monique | |
| dc.creator | Neumann, Doris M. | |
| dc.date | 2002-07-11 | |
| dc.date.accessioned | 2026-07-07T02:04:16Z | |
| dc.date.available | 2026-07-07T02:04:16Z | |
| dc.description | We present the follow-up of three medium redshift galaxy clusters from the SHARC survey observed with XMM-Newton. We studied RX J0256.5+0006 which shows two components which are very likely in interaction. The smallest component exhibits a comet-like structure indicating ram pressure stripping as it falls onto the main cluster. The second cluster, RX J2237.0-1516 is an elliptical cluster with a gas temperature of 3.0$\pm$0.5 keV. The third cluster, RX J1200.8-0328 seems to be in a relaxed state because its shape is regular and we do not see obvious temperature gradient. Its mean temperature is 5.1$^{+0.7}_{-0.5}$ keV. | |
| dc.description | 5 pages; 4 figures; to be published in the Proceedings of the Conference on Matter and Energy in Clusters of Galaxies, Chung-Li (2002), editors: S.Bowyer and C.-Y. Hwang | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0207232 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0207232 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4685 | |
| dc.subject | Astrophysics | |
| dc.title | XMM-Newton AO-1 observations three SHARC galaxy clusters | |
| dc.type | text |