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Elemental abundance analyses with DAO spectrograms - XXI. The hot metallic-lined stars 60 Leonis and 6 Lyrae

dc.contributor.authorCaliskan, H
dc.contributor.authorTektanali, HG
dc.contributor.authorCay, T
dc.contributor.authorKocer, D
dc.contributor.authorAdelman, SJ
dc.date.accessioned2021-03-03T16:14:14Z
dc.date.available2021-03-03T16:14:14Z
dc.date.issued1999
dc.identifier.citationAdelman S., Caliskan H., Cay T., Kocer D., Tektanali H., "Elemental abundance analyses with DAO spectrograms - XXI. The hot metallic-lined stars 60 Leonis and 6 Lyrae", MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.305, sa.3, ss.591-601, 1999
dc.identifier.issn0035-8711
dc.identifier.otherav_4327bd14-548a-4691-87a2-ae186a672279
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/48856
dc.identifier.urihttps://doi.org/10.1046/j.1365-8711.1999.02435.x
dc.description.abstractElemental abundances of the hot metallic-lined (Am) stars 60 Leo and 6 Lyr, with modest rotational velocities, are derived consistently with other studies in this series of papers. Both stars are found to show the Am phenomenon strongly, with nearly solar abundances of the light elements, overabundances of most Fe peak elements, and considerable overabundances of SrYZr, Ba and some rare earths. Ca is underabundant, while Sc is very underabundant.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectFizik
dc.subjectTemel Bilimler
dc.titleElemental abundance analyses with DAO spectrograms - XXI. The hot metallic-lined stars 60 Leonis and 6 Lyrae
dc.typeMakale
dc.relation.journalMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
dc.contributor.department, ,
dc.identifier.volume305
dc.identifier.issue3
dc.identifier.startpage591
dc.identifier.endpage601
dc.contributor.firstauthorID123255


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