IIA Institutional Repository

The lithium in weak G-band stars

Show simple item record

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

Files in this item

This item appears in the following Collection(s)

Show simple item record

Search DSpace


My Account