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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3712
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dc.contributor.authorSagar, R-
dc.contributor.authorBhatt, H. C-
dc.date.accessioned2008-09-17T11:58:56Z-
dc.date.available2008-09-17T11:58:56Z-
dc.date.issued1988-06-
dc.identifier.citationJournal of Astrophysics and Astronomy , Vol. 9, No. 2, pp. 117 - 124en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3712-
dc.description.abstractKinematical distances are estimated for six open star clusters. They agree fairly well with the photometric distances. The kinematical distances cannot, at present, be estimated better than the photometric distances. When more accurate proper motion measurements become available the kinematical distances will improve considerably and may then be used to calibrate the cosmic distance scaleen
dc.language.isoenen
dc.publisherIndian Academy Sciencesen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1988JApA....9..117Sen
dc.subjectAstrometryen
dc.subjectAstronomical Photometryen
dc.subjectBody Kinematicsen
dc.subjectOpen Clustersen
dc.subjectStar Clustersen
dc.subjectStellar Evolutionen
dc.subjectGlobular Clustersen
dc.subjectInterstellar Extinctionen
dc.subjectRadial Velocityen
dc.subjectStellar Motionsen
dc.titleKinematical distances to open star clustersen
dc.typeArticleen
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