New Constraints on the Nuclear Equation of State from the Thermal Emission of Neutron Stars in Quiescent Low-mass X-Ray Binaries

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dc.contributor.authorD'Etivaux, N.B.
dc.contributor.authorGuillot, S.
dc.contributor.authorMargueron, J.
dc.contributor.authorWebb, N.
dc.contributor.authorCatelan, Márcio
dc.contributor.authorReisenegger, Andreas
dc.date.accessioned2020-10-15T20:42:30Z
dc.date.available2020-10-15T20:42:30Z
dc.date.issued2019
dc.format.extent16 páginas
dc.fuente.origenConveris
dc.identifier.doi10.3847/1538-4357/ab4f6c
dc.identifier.issn0004-637X
dc.identifier.urihttps://doi.org/10.3847/1538-4357/ab4f6c
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/47794
dc.issue.numeroNo. 1
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final16
dc.pagina.inicio1
dc.revistaAstrophysical Journales_ES
dc.rightsacceso abierto
dc.titleNew Constraints on the Nuclear Equation of State from the Thermal Emission of Neutron Stars in Quiescent Low-mass X-Ray Binarieses_ES
dc.typeartículo
dc.volumenVol. 887
sipa.codpersvinculados1001556
sipa.codpersvinculados100213
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