An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent
dc.contributor.author | Pietrzynski, G. | |
dc.contributor.author | Minniti, D. | |
dc.date.accessioned | 2016-05-10T18:15:00Z | |
dc.date.available | 2016-05-10T18:15:00Z | |
dc.date.issued | 2013 | |
dc.identifier.doi | 10.1038/nature11878 | |
dc.identifier.issn | 0028-0836 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/13545 | |
dc.identifier.uri | https://doi.org/10.1038/nature11878 | |
dc.language.iso | en | |
dc.relation.isformatof | Nature No. 7439 (495), p. 76-79. | |
dc.revista | Nature | es_ES |
dc.rights | acceso restringido | |
dc.subject.ddc | 520 | |
dc.subject.dewey | Astronomía | es_ES |
dc.subject.other | Binarias eclipsantes | es_ES |
dc.subject.other | Nubes magallánicas | es_ES |
dc.subject.other | Cosmología | es_ES |
dc.subject.other | Galaxias - Mediciones | es_ES |
dc.title | An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent | es_ES |
dc.type | artículo | |
sipa.codpersvinculados | 100504 |
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