Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10694505 | Advances in Space Research | 2005 | 4 Pages |
Abstract
Our XMM-Newton observations of Abell 85 confirm the extended 4Â Mpc filament first detected with ROSAT, which has an X-ray temperature of about â¼2Â keV and is probably made of groups falling on to the cluster. A comparison of the temperature map with numerical simulations show that Abell 85 had intense merging activity in the past and is not fully relaxed, even in the central region. Finally, a deprojected temperature profile has been calculated and used, together with the surface brightness, to estimate the entropy and pressure profiles. Abell 85 only presents a mild flattening of the entropy profile in the center, showing no evidence of an “entropy floor”.
Keywords
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Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Florence Durret, Gastão B. Lima Neto, William Forman,