Integrated parameters of open clusters

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3683

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DC Field	Value	Language
dc.contributor.author	Pandey, A. K	-
dc.contributor.author	Bhatt, B. C	-
dc.contributor.author	Mahra, H. S	-
dc.contributor.author	Sagar, R	-
dc.date.accessioned	2008-09-16T16:19:23Z	-
dc.date.available	2008-09-16T16:19:23Z	-
dc.date.issued	1989-01	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, Vol. 236, No. 1, pp. 263 - 276	en
dc.identifier.issn	0035-8711	-
dc.identifier.uri	http://hdl.handle.net/2248/3683	-
dc.description.abstract	Integrated magnitudes and colors of population I synthetic clusters have been derived using theoretical evolutionary tracks and an age-dependednt initial mass function. A comparison of the theoretically obtained integrated parameters with the observational data of open clusters in the Milky Way and clusters in the LMC has also been made. It is found that the observed dependences show a better agreement with the theoretical dependences obtained in the present work than the theoretical dependences obtained by earlier authors. It is also concluded that the clusters in the LMC in general show a mean reddening of E(B-V) = 0.12 mag.	en
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://ads.ari.uni-heidelberg.de/abs/1989MNRAS.236..263P	en
dc.subject	Open Clusters	en
dc.subject	Star Clusters	en
dc.subject	Magellanic Clouds	en
dc.subject	Milky Way Galaxy	en
dc.subject	Stellar Color	en
dc.subject	Stellar Magnitude	en
dc.title	Integrated parameters of open clusters	en
dc.type	Article	en
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