1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2825
Full metadata record
DC FieldValueLanguage
dc.contributor.authorPandey, A. K-
dc.contributor.authorDurgapal, A. K-
dc.contributor.authorBhatt, B. C-
dc.contributor.authorMohan, V-
dc.contributor.authorMahra, H. S-
dc.date.accessioned2008-07-22T11:50:16Z-
dc.date.available2008-07-22T11:50:16Z-
dc.date.issued1996-
dc.identifier.citationIAU Symposium, No. 174, pp. 339 - 340en
dc.identifier.issn0074-1809-
dc.identifier.urihttp://hdl.handle.net/2248/2825-
dc.description.abstractThe morphological features of CMDs of Be 69 are better understood in terms of convective overshooting.The Comparison of CMDs with the convective overshoot models (Bertelli et al. 1994)produces a good fit for metallicity Z=0.008, age=0.8, 1.0 billion yr and (m-M)=14.3, which corresponds to a distence of 2860 pc.en
dc.format.extent160578 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996IAUS..174..339Pen
dc.subjectCCD photometryen
dc.subjectOpen clustersen
dc.titleCCD Photometry of the Open Cluster BE 69en
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
pandey.pdf156.81 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.