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dc.contributor.authorGulliver, AF
dc.contributor.authorTeker, A
dc.contributor.authorCay, IH
dc.contributor.authorTektunali, GH
dc.contributor.authorKocer, D
dc.contributor.authorCaliskan, H
dc.contributor.authorAdelman, SJ
dc.contributor.authorCay, MT
dc.date.accessioned2021-03-03T10:39:32Z
dc.date.available2021-03-03T10:39:32Z
dc.date.issued2002
dc.identifier.citationCaliskan H., Adelman S., Cay M., Cay I., Gulliver A., Tektunali G., Kocer D., Teker A., "Elemental abundance analyses with DAO spectrograms - XXVI. The superficially normal stars serpentis gamma (F6 V) and 101 Herculis (A7 V)", ASTRONOMY & ASTROPHYSICS, cilt.394, sa.1, ss.187-192, 2002
dc.identifier.issn0004-6361
dc.identifier.otherav_23e913eb-2a74-4d80-b4c4-422b01535a89
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/29062
dc.identifier.urihttps://doi.org/10.1051/0004-6361:20021117
dc.description.abstractElemental abundances analyses of the superfically normal stars gamma Ser (F6 V) and 101 Herculis (A7 V) consistent with previous studies of this series using photographic region spectrograms obtained with Reticon and CCD detectors produced derived values that are generally solar except for Al which is very underabundant and the rare earths which do not have the solar pattern. Similar discrepancies from solar values are seen in other superficially normal stars of this series with similar temperatures. Our results for gamma Ser are in acceptable agreement with other recent studies based on different techniques and spectral regions.
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 - XXVI. The superficially normal stars serpentis gamma (F6 V) and 101 Herculis (A7 V)
dc.typeMakale
dc.relation.journalASTRONOMY & ASTROPHYSICS
dc.contributor.department, ,
dc.identifier.volume394
dc.identifier.issue1
dc.identifier.startpage187
dc.identifier.endpage192
dc.contributor.firstauthorID166223


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