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dc.rights.licensehttp://creativecommons.org/licenses/by-nc-sa/3.0/ve/
dc.contributor.authorMartínez, Justinoes_VE
dc.contributor.authorNúñez, Luises_VE
dc.contributor.authorPavón, Diegoes_VE
dc.date2006-01-26es_VE
dc.date.accessioned2006-01-26T09:00:00Z
dc.date.available2006-01-26T09:00:00Z
dc.date.created1994-01-01es_VE
dc.date.issued2006-01-26T09:00:00Zes_VE
dc.identifier.otherT016300002559/0es_VE
dc.identifier.urihttp://www.saber.ula.ve/handle/123456789/16846
dc.description.abstractRadiation flow and viscous stresses in anisotropic gravitational collapse (Martínez, Justino; Pavón, Diego; Núñez, Luis) Abstract The Herrera-Jimenez-Ruggeri method is employed to analyse the evolution of anisotropic radiating fluid spheres endowed with viscous stresses. The growth of the anisotropy with the distance to the centre allows us to divide the sphere interior into three concentric zones, which differ from each other in the degree of interaction between matter and radiation. The compression wave plays a greater role in the dynamics than it does in the isotropic case. Other effects are also considered in detail. Artículo publicado en: Mon. Not. R. Astron. Soc. 271, 463-475 (1994).es_VE
dc.format.extent1821365es_VE
dc.language.isoeses_VE
dc.publisherSABER ULAes_VE
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectDistribuciones autogravitanteses_VE
dc.titleRadiation flow and viscous stresses in anisotropic gravitational collapsees_VE
dc.typeinfo:eu-repo/semantics/article
dc.description.emailnunez@ula.vees_VE
dc.description.tiponivelNivel monográficoes_VE
dc.subject.facultadFacultad de Ciencias.es_VE
dc.subject.keywordsGravitation hydrodynamicses_VE
dc.subject.keywordsRadiative transferes_VE
dc.subject.keywordsRelativityes_VE
dc.subject.keywordsStars: masslosses_VE
dc.subject.keywordsStars: neutrones_VE
dc.subject.laboratorioLaboratorio de Física Teóricaes_VE
dc.subject.tipoArtículoses_VE


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