The relation between the most-massive star and its parental star cluster mass

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dc.contributor.authorWeidner, Carsten
dc.date.accessioned10-05-2016 15:14
dc.date.available10-05-2016 15:14
dc.date.issued2010
dc.identifier.doi10.1111/j.1365-2966.2009.15633.x
dc.identifier.issn0035-8711
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/13521
dc.identifier.urihttps://doi.org/10.1111/j.1365-2966.2009.15633.x
dc.identifier.wosidWOS:000272867100040
dc.language.isoen
dc.nota.accesoContenido completo
dc.relation.isformatofMonthly Notices of the Royal Astronomical Society No. 1 (401), p. 275-293.
dc.revistaMonthly Notices of the Royal Astronomical Society
dc.subject.ddc520
dc.subject.deweyAstronomía
dc.subject.otherFormación de Galaxias
dc.subject.otherEstrellas - Cúmulos
dc.subject.otherEstrellas - Masas
dc.titleThe relation between the most-massive star and its parental star cluster mass
dc.typeartículo
sipa.codpersvinculados1004673
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