A comparison of optical and near-infrared colours of Magellanic Cloud star clusters with predictions of simple stellar population models

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dc.contributor.authorPessev P
dc.contributor.authorPuzia, Thomas H.
dc.date.accessioned2017-04-12T13:10:29Z
dc.date.available2017-04-12T13:10:29Z
dc.date.issued2008
dc.identifier.doi10.1111/j.1365-2966.2008.12935.x
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1111/j.1365-2966.2008.12935.x
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/19346
dc.language.isoen
dc.relation.isformatofMonthly Notices of the Royal Astronomical Society. Vol. 385, no. 3 (2008), p. [1535]-1560
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherNubes magallánicases_ES
dc.subject.otherEstrellas - Cúmuloses_ES
dc.subject.otherFotometría astronómicaes_ES
dc.titleA comparison of optical and near-infrared colours of Magellanic Cloud star clusters with predictions of simple stellar population modelses_ES
dc.typeartículo
sipa.codpersvinculados1008925
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