Effects of spot structure of lines of rare earths and non-LTE effects on lithium abundance estimates for two roAp stars

dc.contributor.author	Mashonkina L.
dc.contributor.author	Shavrina A.
dc.contributor.author	Khalack V.
dc.contributor.author	Polosukhina N.
dc.contributor.author	Tsymbal V.
dc.contributor.author	Vygonets V.
dc.date.accessioned	2018-09-17T21:10:23Z
dc.date.available	2018-09-17T21:10:23Z
dc.date.issued	2002
dc.identifier.issn	1063-7729
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/134622
dc.description.abstract	Taking into account blending of the lithium 6108 Å line profile by adjacent rare-earth lines together with their spotted surface structure does not appreciably affect lithium abundance estimates for the atmospheres of HD 83368 and HD 60435 but provides a better fit of the observed and stimulated line profiles. Our computed non-LTE corrections reduce the lithium abundance estimates by 0.1-0.2 dex for both stars. Given the uncertainties in the lithium abundances, it is not possible to be certain whether the lithium abundances in map stars, or at least in their spots, exceed the cosmic (primordial) value. © 2002 MAIK "Nauka/Interperiodica".
dc.relation.ispartofseries	Astronomy Reports
dc.title	Effects of spot structure of lines of rare earths and non-LTE effects on lithium abundance estimates for two roAp stars
dc.type	Article
dc.relation.ispartofseries-issue	1
dc.relation.ispartofseries-volume	46
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	27
dc.source.id	SCOPUS10637729-2002-46-1-SID0036001517

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