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The dust emission SED of X-ray emitting regions in Stephan's Quintet

dc.contributor.authorNatale, G.
dc.contributor.authorTuffs, Richard J.
dc.contributor.authorXu, C. K.
dc.contributor.authorPopescu, Cristina C.
dc.contributor.authorFischera, J.
dc.contributor.authorLisenfeld , Ute 
dc.contributor.authorLu, N.
dc.contributor.authorAppleton, P. N.
dc.contributor.authorDopita, M.
dc.contributor.authorDuc, P.-A.
dc.contributor.authorGao, Y.
dc.contributor.authorReach, W.
dc.contributor.authorSulentic, J.
dc.contributor.authorYun, M. S.
dc.date.accessioned2013-10-08T07:49:17Z
dc.date.available2013-10-08T07:49:17Z
dc.date.issued2012
dc.identifier.citationNatale, G.; et al. The dust emission SED of X-ray emitting regions in Stephan's Quintet. Proceedings of the International Astronomical Union, 7(S284): 337-341 (2011). [http://hdl.handle.net/10481/28342]es_ES
dc.identifier.issn1743-9213
dc.identifier.issn1743-9221
dc.identifier.otherdoi: 10.1017/S1743921312009374
dc.identifier.otherarXiv:1203.3430v1
dc.identifier.urihttp://hdl.handle.net/10481/28342
dc.descriptionConference proceedings IAU Symposium 284 "The Spectral energy distribution of galaxies", 5-9 September 2011, Preston, UK.es_ES
dc.description.abstractWe analysed the Spitzer maps of Stephan's Quintet in order to investigate the nature of the dust emission associated with the X-ray emitting regions of the large scale intergalactic shock and of the group halo. This emission can in principle be powered by dust-gas particle collisions, thus providing efficient cooling of the hot gas. However the results of our analysis suggest that the dust emission from those regions is mostly powered by photons. Nonetheless dust collisional heating could be important in determining the cooling of the IGM gas and the large scale star formation morphology observed in SQ.es_ES
dc.language.isoenges_ES
dc.publisherInternational Astronomical Uniones_ES
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs 3.0 Licensees_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es_ES
dc.subjectGalaxies es_ES
dc.subjectInteractionses_ES
dc.subjectIntergalactic mediumes_ES
dc.subjectInfraredes_ES
dc.subjectHCG92es_ES
dc.titleThe dust emission SED of X-ray emitting regions in Stephan's Quintetes_ES
dc.typepreprintes_ES
dc.rights.accessRightsopen accesses_ES


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