Near infrared photometry of the young clusters NGC 1960, NGC 2453 and NGC 2384

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/786

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DC Field	Value	Language
dc.contributor.author	Hasan, P	-
dc.date.accessioned	2006-03-15T04:36:14Z	-
dc.date.available	2006-03-15T04:36:14Z	-
dc.date.issued	2005-09	-
dc.identifier.citation	BASI, Vol. 33, No. 3, pp. 311-315	en
dc.identifier.uri	http://hdl.handle.net/2248/786	-
dc.description.abstract	Infrared observations of young star clusters provide vital clues to the star formation process and evolution of stars. This brief report on my thesis gives a brief description of the observations and analysis of the young star clusters NGC 1960, NGC 2453 and NGC 2384 observed in the near infrared bands at the Mt Abu Infrared Observatory, Gurushikhar in February 2000. Estimates of distance and age for these clusters for the first time using JHK data have been obtained. The colourmagnitude diagrams of these clusters have been extended to the fainter end as far as possible. The observed data was compared to that obtained by 2MASS. A more detailed paper will be published elsewhere	en
dc.format.extent	206299 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	NIR photometry	en
dc.subject	star - clusters colour-magnitude diagrams -2MASS	en
dc.title	Near infrared photometry of the young clusters NGC 1960, NGC 2453 and NGC 2384	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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