dc.creatorFalcón Veloz, Nelson Leonardo
dc.date.accessioned2015-06-24T01:25:09Z
dc.date.accessioned2022-12-14T14:17:10Z
dc.date.available2015-06-24T01:25:09Z
dc.date.available2022-12-14T14:17:10Z
dc.date.created2015-06-24T01:25:09Z
dc.date.issued2004
dc.identifierSatellites and Tidal Streams ASP Conference Series, Vol. 327, 2004
dc.identifier1-58381-190-7
dc.identifierhttp://hdl.handle.net/123456789/1752
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5349431
dc.description.abstractWe have been examining the role of heat conduction during the streams and other transitory event in the inner atmosphere of clusters of galaxies. Assuming the propagation of heat by thermal waves and hydrostatic equilibrium, we show that the conduction cooling timescale could be different from simple heat conduction. The implications for X-ray observations and interferometry are discussed
dc.languagees_ES
dc.publisherAstronomical Society of the Pacific
dc.relationVolume 327, 2004;
dc.subjectHydrostatic equilibrium
dc.subjectClusters of galaxies
dc.subjectThermal cconduction
dc.subjectCooling
dc.titleCooling and thermal conduction in clusters of galaxies
dc.typeArticle


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