Near-infrared adaptive optics imaging of infrared luminous galaxies: the brightest cluster magnitude-star formation rate relation

dc.date.accessioned2016-11-29T20:51:52Z
dc.date.available2016-11-29T20:51:52Z
dc.date.created2016-11-29T20:51:52Z
dc.date.issued2013
dc.identifier2041-8205
dc.identifierhttp://hdl.handle.net/10533/133848
dc.identifier1130458
dc.identifierWOS:000324626700005
dc.identifier2041-8213
dc.languageeng
dc.publisherIOP PUBLISHING LTD
dc.relationhttps://doi.org/10.1088/2041-8205/775/2/L38
dc.relation10.1088/2041-8205/775/2/L38
dc.relation10.1088/2041-8205/775/2/L38
dc.relationinfo:eu-repo/grantAgreement/Fondecyt/1130458
dc.relationinfo:eu-repo/semantics/dataset/hdl.handle.net/10533/93477
dc.relationinstname: Conicyt
dc.relationreponame: Repositorio Digital RI2.0
dc.relationinstname: Conicyt
dc.relationreponame: Repositorio Digital RI2.0
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleNear-infrared adaptive optics imaging of infrared luminous galaxies: the brightest cluster magnitude-star formation rate relation
dc.typeArticulo


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