An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent

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dc.contributor.authorPietrzynski, G.
dc.contributor.authorMinniti, D.
dc.date.accessioned2016-05-10T18:15:00Z
dc.date.available2016-05-10T18:15:00Z
dc.date.issued2013
dc.identifier.doi10.1038/nature11878
dc.identifier.issn0028-0836
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/13545
dc.identifier.urihttps://doi.org/10.1038/nature11878
dc.language.isoen
dc.relation.isformatofNature No. 7439 (495), p. 76-79.
dc.revistaNaturees_ES
dc.rightsacceso restringido
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherBinarias eclipsanteses_ES
dc.subject.otherNubes magallánicases_ES
dc.subject.otherCosmologíaes_ES
dc.subject.otherGalaxias - Medicioneses_ES
dc.titleAn eclipsing-binary distance to the Large Magellanic Cloud accurate to two per centes_ES
dc.typeartículo
sipa.codpersvinculados100504
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