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Mass function study of six open clusters Be 10, Be 67,To 5, Be 15, Be 71 and King 1

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dc.contributor.author Lata, S
dc.date.accessioned 2006-03-14T04:54:26Z
dc.date.available 2006-03-14T04:54:26Z
dc.date.issued 2005-06
dc.identifier.citation BASI, Vol. 33, No. 2, pp. 51-66 en
dc.identifier.uri http://hdl.handle.net/2248 /752
dc.description.abstract In the present study, we have used the CCD data to determine the luminosity and mass function of six open clusters. Members of clusters are identified using photometric and statistical criteria. From these members, we have derived luminosity functions and determined the mass function slopes for the clusters under study. The mass function slopes for clusters Be 10, Be 67, To 5, Be 15, Be 71 and King 1 are 1.39(+/-)0.73, 3.41(+/-)0.98, 1.32(+/-)0.47, 1.35(+/-)0.46, 3.02(+/-)0.81 and 1.46(+/-)0.71 respectively. These slopes agree with the Salpeter value (x=1.35) within errors except for clusters Be 67 and Be 71 which have steeper slopes. The clusters Be 10, Be 67, To 5 and Be 15 show mass segregation while King 1 gives weak evidence of mass segregation and Be 71 does not show the ects of mass segregation. All the clusters under study are dynamically relaxed en
dc.format.extent 453046 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.subject Stars: luminosity function, mass function en
dc.subject open clusters and associations en
dc.title Mass function study of six open clusters Be 10, Be 67,To 5, Be 15, Be 71 and King 1 en
dc.type Article en


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