dc.creatorGUILLERMO TENORIO TAGLE
dc.creatorSERGIY SILICH
dc.date2009
dc.date.accessioned2023-07-25T16:23:33Z
dc.date.available2023-07-25T16:23:33Z
dc.identifierhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1379
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7806575
dc.descriptionIn this work, we present a comprehensive X-ray picture of the interaction between a super star cluster and the interstellar medium. In order to do that, we compare and combine the X-ray emission from the superwind driven by the cluster with the emission from the windblown bubble. Detailed analytical models for the hydrodynamics and X-ray luminosity of fast polytropic superwinds are presented. The superwind X-ray luminosity models are an extension of the results obtained in Paper I. Here, the superwind polytropic character allows us to parametrize a wide variety of effects, for instance, radiative cooling. Additionally, X-ray properties that are valid for all bubble models taking thermal evaporation into account are derived. The final X-ray picture is obtained by calculating analytically the expected surface brightness and weighted temperature of each component. All of our X-ray models have an explicit dependence on metallicity and admit general emissivities as functions of the hydrodynamical variables. We consider a realistic X-ray emissivity that separates the contributions from hydrogen and metals. The paper ends with a comparison of the models with observational data.
dc.formatapplication/pdf
dc.languageeng
dc.publisherMonthly Notices of the Royal Astronomical Society
dc.relationcitation:Añorve Zeferino, G. A., et al., (2009). On the X-ray emission from massive star clusters and their evolving superbubbles – II. Detailed analytics and observational effects, Monthly Notices of the Royal Astronomical Society. Vol. 394, 1284–1306
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0
dc.subjectinfo:eu-repo/classification/Inspec/Hydrodynamics
dc.subjectinfo:eu-repo/classification/Inspec/Stars: winds, outflows
dc.subjectinfo:eu-repo/classification/Inspec/ISM: bubbles
dc.subjectinfo:eu-repo/classification/Inspec/X-rays: ISM.
dc.subjectinfo:eu-repo/classification/cti/1
dc.subjectinfo:eu-repo/classification/cti/21
dc.subjectinfo:eu-repo/classification/cti/21
dc.titleOn the X-ray emission from massive star clusters and their evolving superbubbles – II. Detailed analytics and observational effects
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/acceptedVersion
dc.audiencestudents
dc.audienceresearchers
dc.audiencegeneralPublic


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