Recent CHANDRA and XMM observations of two very different galaxy clusters: RBS797 and CL 0939+4713
| dc.creator | De Filippis, E. | |
| dc.creator | Schindler, S. | |
| dc.creator | Castillo-Morales, A. | |
| dc.date | 2002-01-21 | |
| dc.date.accessioned | 2026-07-07T02:02:18Z | |
| dc.date.available | 2026-07-07T02:02:18Z | |
| dc.description | RBS797 and CL 0939+4713 are two intermediate red-shift clusters ($z=0.35-0.41$). They have very different morphologies but both show surprisingly interesting structures. RBS797 looks relaxed, with an almost circular morphology; a CHANDRA observation of this cluster has revealed two deep depressions in the X-ray emission near the core. CL 0939+4713 has instead an irregular morphology with evident substructures which seem to be in the process of merging. | |
| dc.description | 6 pages; Proccedings of the Symposium "New Visions of the X-ray Universe in the XMM-Newton and Chandra era", Noordwijk, November 2001 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0201349 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0201349 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4040 | |
| dc.subject | Astrophysics | |
| dc.title | Recent CHANDRA and XMM observations of two very different galaxy clusters: RBS797 and CL 0939+4713 | |
| dc.type | text |