Constraining Dense Matter Superfluidity Through Thermal Emission From Millisecond Pulsars

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dc.contributor.authorReisenegger, Andreas
dc.date.accessioned2017-04-12T13:10:39Z
dc.date.available2017-04-12T13:10:39Z
dc.date.issued1997
dc.identifier.doi10.1086/304417
dc.identifier.issn0004-637X
dc.identifier.urihttps://doi.org/10.1086/304417
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/19423
dc.language.isoen
dc.relation.isformatofAstrophysical Journal. Vol. 485, no. 1 (1997), p. [313]-318
dc.revistaAstrophysical Journales_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas de neutroneses_ES
dc.subject.otherPulsareses_ES
dc.subject.otherMateria condensadaes_ES
dc.subject.otherAstronomía de rayos Xes_ES
dc.titleConstraining Dense Matter Superfluidity Through Thermal Emission From Millisecond Pulsarses_ES
dc.typeartículo
sipa.codpersvinculados100213
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