K-Band Red Clump Distance to the Large Magellanic Cloud

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dc.contributor.authorAlves D
dc.contributor.authorMinniti, D.
dc.date.accessioned2017-04-10T18:36:35Z
dc.date.available2017-04-10T18:36:35Z
dc.date.issued2002
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/17492
dc.language.isoen
dc.relation.isformatofAstrophysical Journal. Vol. 573, no. 1 (2002), p. [L51]-L54
dc.revistaAstrophysical Journales_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas variableses_ES
dc.subject.otherNubes magallánicasAstronomía infrarrojaes_ES
dc.titleK-Band Red Clump Distance to the Large Magellanic Cloudes_ES
dc.typeartículo
sipa.codpersvinculados100504
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