XMM-Newton temperature maps for five intermediate redshift clusters of galaxies

Simple item page
dc.creatorDurret, Florence
dc.creatorNeto, Gastao B. Lima
dc.date2007-07-27
dc.date.accessioned2026-07-07T11:41:38Z
dc.date.available2026-07-07T11:41:38Z
dc.descriptionWe have analyzed XMM-Newton archive data for five clusters of galaxies (redshifts 0.223 to 0.313) covering a wide range of dynamical states, from relaxed objects to clusters undergoing several mergers. We present here temperature maps of the X-ray gas together with a preliminary interpretation of the formation history of these clusters.
dc.description4 pages, 2 figs. Accepted for publication in the Proceedings of the 36th COSPAR Scientific Assembly
dc.identifierhttps://arxiv.org/abs/0707.4120
dc.identifierhttp://arxiv.org/abs/0707.4120
dc.identifierAdv.SpaceRes.42:578-580,2008
dc.identifierdoi:10.1016/j.asr.2007.07.033
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200604
dc.subjectAstrophysics
dc.titleXMM-Newton temperature maps for five intermediate redshift clusters of galaxies
dc.typetext

Files

Collections

arXiv