dc.creator | GUILLERMO TENORIO TAGLE | |
dc.creator | SERGIY SILICH | |
dc.date | 2009 | |
dc.date.accessioned | 2023-07-25T16:23:33Z | |
dc.date.available | 2023-07-25T16:23:33Z | |
dc.identifier | http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1379 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7806575 | |
dc.description | In 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.format | application/pdf | |
dc.language | eng | |
dc.publisher | Monthly Notices of the Royal Astronomical Society | |
dc.relation | citation: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.rights | info:eu-repo/semantics/openAccess | |
dc.rights | http://creativecommons.org/licenses/by-nc-nd/4.0 | |
dc.subject | info:eu-repo/classification/Inspec/Hydrodynamics | |
dc.subject | info:eu-repo/classification/Inspec/Stars: winds, outflows | |
dc.subject | info:eu-repo/classification/Inspec/ISM: bubbles | |
dc.subject | info:eu-repo/classification/Inspec/X-rays: ISM. | |
dc.subject | info:eu-repo/classification/cti/1 | |
dc.subject | info:eu-repo/classification/cti/21 | |
dc.subject | info:eu-repo/classification/cti/21 | |
dc.title | On the X-ray emission from massive star clusters and their evolving superbubbles – II. Detailed analytics and observational effects | |
dc.type | info:eu-repo/semantics/article | |
dc.type | info:eu-repo/semantics/acceptedVersion | |
dc.audience | students | |
dc.audience | researchers | |
dc.audience | generalPublic | |