The lithium in weak G-band stars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4136

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DC Field	Value	Language
dc.contributor.author	Parthasarathy, M	-
dc.contributor.author	Kameswara Rao, N	-
dc.date.accessioned	2008-12-19T10:39:20Z	-
dc.date.available	2008-12-19T10:39:20Z	-
dc.date.issued	1980-11	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 73, No. 1, pp. 251 - 257	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2248/4136	-
dc.description.abstract	The lithum abundance in weak G-band stars is found to be linearly correlated with CH deficiency. Weak G-band stars with a high Li abundance are found to show relatively least carbon deficiency, while the stars with a relatively low Li abundance show a high under-abundance of carbon.	en
dc.language.iso	en	en
dc.publisher	D. Reidel Publishing Co.	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1980Ap%26SS..73..251P	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00642380	en
dc.subject	Carbon	en
dc.subject	Lithium	en
dc.subject	Main Sequence Stars	en
dc.subject	Stellar Spectra:Abundance	en
dc.subject	Globular Clusters:Nitrogen	en
dc.title	The lithium in weak G-band stars	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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