dc.contributorSERGIY SILICH
dc.contributorGUILLERMO TENORIO TAGLE
dc.creatorFILIBERTO HUEYOTL ZAHUANTITLA
dc.date2010-09
dc.date.accessioned2023-07-25T16:21:46Z
dc.date.available2023-07-25T16:21:46Z
dc.identifierhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/517
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7805735
dc.descriptionThe results of this thesis leads to an intrinsic link between the luminosity of a SMBH located at the center of a young nuclear starburst and the starburst parameters. However, the model here developed still does not include some potentially important physical ingredients and thus requires further improvement. So far we have assumed that stars are equally distributed within the star-forming region. Therefore, a more realistic model for the stellar density distribution has to be developed, as it was suggested by some authors (see, Rodriguez-González et al. 2007) who have considered relatively low mass stellar clusters and presented the results without accounting for the impact of gravity provided by the stellar component and the presence of the central black hole.
dc.formatapplication/pdf
dc.languageeng
dc.publisherInstituto Nacional de Astrofísica, Óptica y Electrónica
dc.relationcitation:Hueyotl-Zahuantitla F.
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0
dc.subjectinfo:eu-repo/classification/Galaxias activas/Active galaxies
dc.subjectinfo:eu-repo/classification/Agujeros negros/Black holes
dc.subjectinfo:eu-repo/classification/Acreción/Accretion
dc.subjectinfo:eu-repo/classification/Formación de estrellas/Star formation
dc.subjectinfo:eu-repo/classification/Starburst galaxies/Starburst galaxies
dc.subjectinfo:eu-repo/classification/Dinámica de fluidos astrofísicos/Astrophysical fluid dynamics
dc.subjectinfo:eu-repo/classification/cti/1
dc.subjectinfo:eu-repo/classification/cti/21
dc.subjectinfo:eu-repo/classification/cti/21
dc.titleSpherically symmetric accretion from a nuclear young starburst onto a super massive black hole
dc.typeinfo:eu-repo/semantics/doctoralThesis
dc.typeinfo:eu-repo/semantics/acceptedVersion
dc.audiencestudents
dc.audienceresearchers
dc.audiencegeneralPublic


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