The atmospheric lithium abundances of solar analogues

dc.contributor.author	Galeev A.
dc.contributor.author	Bikmaev I.
dc.contributor.author	Mashonkina L.
dc.contributor.author	Musaev F.
dc.contributor.author	Galazutdinov G.
dc.date.accessioned	2018-09-17T21:10:47Z
dc.date.available	2018-09-17T21:10:47Z
dc.date.issued	2004
dc.identifier.issn	1063-7729
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/134633
dc.description.abstract	We have analyzed the lithium abundance in the atmospheres of 20 stars that are solar analogues based on high-resolution echelle spectra using model atmospheres in a non-LTE approach. In terms of their lithium abundances, the stars (which are located in a narrow range of temperatures of 5650-5900 K) can be divided into two groups: one with low lithium abundances, as in the solar atmosphere, and one with lithium abundances that are higher than the solar value by about 1 dex (with the accuracy of the lithium abundances being 0.15 dex). © 2004 MAIK "Nauka/Interperiodica".
dc.relation.ispartofseries	Astronomy Reports
dc.title	The atmospheric lithium abundances of solar analogues
dc.type	Article
dc.relation.ispartofseries-issue	6
dc.relation.ispartofseries-volume	48
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	511
dc.source.id	SCOPUS10637729-2004-48-6-SID3543042490

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