Показать сокращенную информацию
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 |