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dc.provenanceComisión de Investigaciones Científicas-
dc.contributorBenvenuto, Omar Gustavo-
dc.contributorDe Vito, María Alejandra-
dc.creatorBenvenuto, Omar Gustavo-
dc.creatorDe Vito, María Alejandra-
dc.date2012-07-
dc.date.accessioned2019-04-29T16:03:01Z-
dc.date.available2019-04-29T16:03:01Z-
dc.date.issued2012-07-
dc.identifierhttp://digital.cic.gba.gob.ar/handle/11746/4225-
dc.identifierDocumento completo-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/307885-
dc.descriptionThe existence of millisecond pulsars with planet-mass companions in close orbits is challenging from the stellar evolution point of view. We calculate in detail the evolution of binary systems self-consistently, including mass transfer, evaporation, and irradiation of the donor by X-ray feedback, demonstrating the existence of a new evolutionary path leading to short periods and compact donors as required by the observations of PSR J1719-1438. We also point out the alternative of an exotic nature of the companion planet-mass star.-
dc.formatapplication/pdf-
dc.format18 p.-
dc.languageeng-
dc.publisherIOPscience-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightsAttribution 4.0 International (BY 4.0)-
dc.sourcereponame:CIC Digital (CICBA)-
dc.sourceinstname:Comisión de Investigaciones Científicas de la Provincia de Buenos Aires-
dc.sourceinstacron:CICBA-
dc.source.urihttp://digital.cic.gba.gob.ar/handle/11746/4225-
dc.source.uriDocumento completo-
dc.subjectAstronomía-
dc.titleEvolutionary trajectories of ultra-compact "black widow" pulsars with very low mass companions-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/submittedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
Aparece en las colecciones: Comisión de Investigaciones Científicas de la Prov. de Buenos Aires

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