The Gap in the H-R Diagram of Open Clusters with Special Reference to NGC 2169, NGC 1778 and Tr I

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/553

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DC Field	Value	Language
dc.contributor.author	Sagar, R	-
dc.contributor.author	Joshi, U. C	-
dc.date.accessioned	2005-08-19T03:54:29Z	-
dc.date.available	2005-08-19T03:54:29Z	-
dc.date.issued	1978-06	-
dc.identifier.citation	BASI, Vol. 6, No. 2, pp. 37-41	en
dc.identifier.uri	http://hdl.handle.net/2248/553	-
dc.description.abstract	The colour-magnitude diagrams of the open clusters NGC 1778 and Tr I indicate the presence of gaps on the rising branches of the evolving main sequnces. The positions of these gaps are compared with those found in other clusters and the effect of evolution on the position of the gap is discussed. The initial luminosity functions of these clusters as also for NGC 2169, closely fit the respective cluster luminosity functions	en
dc.format.extent	605905 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Astronomical Society of India	en
dc.subject	NGC 2169	en
dc.subject	NGC 1778	en
dc.title	The Gap in the H-R Diagram of Open Clusters with Special Reference to NGC 2169, NGC 1778 and Tr I	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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