Rotochemical Heating in Millisecond Pulsars: Formalism and Nonsuperfluid Case

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dc.contributor.authorFernández, R.
dc.contributor.authorReisenegger, Andreas
dc.date.accessioned2017-04-11T14:43:35Z
dc.date.available2017-04-11T14:43:35Z
dc.date.issued2005
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/18617
dc.language.isoen
dc.relation.isformatofAstrophysical Journal. Vol. 625, no. 1 (2005), p. [291]-306
dc.revistaAstrophysical Journales_ES
dc.rightsacceso restringido
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas de neutroneses_ES
dc.subject.otherEstrella -s Rotaciónes_ES
dc.subject.otherPulsareses_ES
dc.titleRotochemical Heating in Millisecond Pulsars: Formalism and Nonsuperfluid Casees_ES
dc.typeartículo
sipa.codpersvinculados100213
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