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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/950
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dc.contributor.authorSagar, R-
dc.contributor.authorBhatt, H. C-
dc.date.accessioned2006-04-12T06:02:51Z-
dc.date.available2006-04-12T06:02:51Z-
dc.date.issued1989-03-
dc.identifier.citationBASI, Vol. 17, No. 1 & 2, pp. 1-5en
dc.identifier.urihttp://hdl.handle.net/2248/950-
dc.description.abstractProper motion measurements are used to study the internal kinematics in the open star clusters NGC 654 and 6087. It is found that intrinsic dispersions are independent of stellar mass and radial distance in both clusters. Consideration is given to the velocity isotropy observed in both clustersen
dc.format.extent377096 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indianen
dc.subjectInternal motionen
dc.subjectOpen clusteren
dc.subjectStellar dynamicsen
dc.titleInternal motions in the open star clusters NGC 654 and 6087en
dc.typeArticleen
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