Dusty super star cluster winds: their impact on the interstellar medium and infrared manifestations

dc.creatorSERGIO MARTINEZ GONZALEZ
dc.date2015-12-11
dc.date.accessioned2023-07-25T16:20:42Z
dc.date.available2023-07-25T16:20:42Z
dc.identifierhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/19
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7805242
dc.descriptionIn light of the growing evidence pointing at core-collapse supernovae as large dust producers, and given their immense number in young massive stellar clusters (SSCs), this work is devoted to address the influence of stochastic injection, sputtering and outflow of dust grains on their emission properties inside the hot and dense intracluster medium. The theory of dust radiative cooling, which considers time-dependent dust size distributions and chemical composition, is combined with a self-consistent semi-analytic method, in order to study the hydrodynamics of spherically symmetric winds driven by SSCs with a generalized Schuster stellar density profile.
dc.formatapplication/pdf
dc.languageeng
dc.publisherInstituto Nacional de Astrofísica, Óptica y Electrónica
dc.relationcitation:Martinez-Gonzalez S.
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0
dc.subjectinfo:eu-repo/classification/Hidrodinámica/Hydrodinamics
dc.subjectinfo:eu-repo/classification/Estrella/Star clusters
dc.subjectinfo:eu-repo/classification/Estelar/Stellar winds
dc.subjectinfo:eu-repo/classification/Polvo cósmico/Cosmic dust
dc.subjectinfo:eu-repo/classification/Medio/Interstellar medium
dc.subjectinfo:eu-repo/classification/cti/1
dc.subjectinfo:eu-repo/classification/cti/21
dc.subjectinfo:eu-repo/classification/cti/2105
dc.subjectinfo:eu-repo/classification/cti/2105
dc.titleDusty super star cluster winds: their impact on the interstellar medium and infrared manifestations
dc.typeinfo:eu-repo/semantics/doctoralThesis
dc.audiencegeneralPublic


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