The lithium in weak G-band stars

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