Rotochemical heating of millisecond and classical pulsars with anisotropic and density-dependent superfluid gap models

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dc.contributor.authorGonzález Jiménez, Nicolás
dc.contributor.authorPetrovich Balbontín, Cristóbal
dc.contributor.authorReisenegger, Andreas
dc.date.accessioned2016-05-10T18:14:55Z
dc.date.available2016-05-10T18:14:55Z
dc.date.issued2015
dc.identifier.issn0035-8711
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/13496
dc.identifier.urihttps://doi.org/10.1093/mnras/stu2558
dc.language.isoen
dc.nota.accesocontenido completo
dc.relation.isformatofMonthly Notices of the Royal Astronomical Society Vol. 447, No. 3, p. 2073-2084.
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas de neutroneses_ES
dc.subject.otherEstrellas - Rotaciónes_ES
dc.subject.otherPulsareses_ES
dc.titleRotochemical heating of millisecond and classical pulsars with anisotropic and density-dependent superfluid gap modelses_ES
dc.typeartículo
dc.volumenVol. 447
sipa.codpersvinculados100213
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