Evolutionary trajectories of ultra-compact "black widow" pulsars with very low mass companions

cic.isFulltexttruees
cic.isPeerReviewedtruees
cic.lugarDesarrolloUniversidad Nacional de La Plata es
cic.versioninfo:eu-repo/semantics/submittedVersiones
dc.date.accessioned2016-09-14T15:06:56Z
dc.date.available2016-09-14T15:06:56Z
dc.identifier.urihttps://digital.cic.gba.gob.ar/handle/11746/4225
dc.titleEvolutionary trajectories of ultra-compact "black widow" pulsars with very low mass companionsen
dc.typeArtículoes
dcterms.abstractThe 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.en
dcterms.creator.authorBenvenuto, Omar Gustavoes
dcterms.creator.authorDe Vito, María Alejandraes
dcterms.extent18 p.es
dcterms.identifier.otherDOI:10.1088/2041-8205/753/2/L33es
dcterms.identifier.urlDocumento completoes
dcterms.isPartOf.issuevol. 753es
dcterms.isPartOf.seriesThe Astrophysical Journal Letterses
dcterms.issued2012-07
dcterms.languageIngléses
dcterms.licenseAttribution 4.0 International (BY 4.0)es
dcterms.publisherIOPsciencees
dcterms.subject.materiaAstronomíaes

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