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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3670
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dc.contributor.authorSagar, R-
dc.contributor.authorMiakutin, V. I-
dc.contributor.authorPiskunov, A. E-
dc.contributor.authorDluzhnevskaia, O. B-
dc.date.accessioned2008-09-16T15:58:23Z-
dc.date.available2008-09-16T15:58:23Z-
dc.date.issued1988-10-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 234, No. 4, pp. 831 - 845en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/3670-
dc.description.abstractThe stellar spatial distribution is studied as a function of mass in 11 young open clusters. In seven of these clusters, mass segregation is observed. The possibility of two cluster centers for NGC 2264 is discussed. It is found that the mass segregation may by due to star formation. It is suggested that the observed mass segregation in open clusters older than some million years might be due to a combination of both initial star formation conditions and dynamical evolutionary processes, whereas only initial star formation conditions are responsible for mass segregation in younger clusters.en
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1988MNRAS.234..831Sen
dc.subjectMass Distributionen
dc.subjectOpen Clustersen
dc.subjectSpatial Distributionen
dc.subjectStar Distributionen
dc.subjectStellar Massen
dc.subjectCosmologyen
dc.subjectStar Formationen
dc.subjectStellar Evolutionen
dc.subjectStellar Motionsen
dc.titleA study of the spatial stellar mass distribution in some young open clustersen
dc.typeArticleen
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