XMM-Newton and Chandra view of the Cluster Abell 85 and its X-Ray Filament
| dc.creator | Neto, Gastao B. Lima | |
| dc.creator | Durret, Florence | |
| dc.date | 2002-07-17 | |
| dc.date.accessioned | 2026-07-07T02:04:21Z | |
| dc.date.available | 2026-07-07T02:04:21Z | |
| dc.description | From ROSAT data, the bright X-ray cluster Abell 85 was found to show a roughly symmetrical shape, on to which are superimposed several features, among which: (1) a blob or group of galaxies falling on to the main cluster, with the gas in the impact region probably hotter and the galaxies in that zone showing enhanced star formation; (2) a filament, either diffuse or made of small groups of galaxies, extending at least 4 Mpc from the cluster (Durret et al. 1998). Preliminary results obtained from XMM-Newton and Chandra observations of Abell 85 and its filament will be presented. | |
| dc.description | Poster paper presented at the conference ``Matter and Energy in Clusters of Galaxies'', Taiwan April 23-27, 2002, Chorng-Yuan Hwang and Stuart Bowyer, Eds | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0207362 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0207362 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4719 | |
| dc.subject | Astrophysics | |
| dc.title | XMM-Newton and Chandra view of the Cluster Abell 85 and its X-Ray Filament | |
| dc.type | text |