| dc.contributor.author | BOLCAL, C | |
| dc.contributor.author | ADELMAN, SJ | |
| dc.contributor.author | KOCER, D | |
| dc.date.accessioned | 2021-03-04T19:24:04Z | |
| dc.date.available | 2021-03-04T19:24:04Z | |
| dc.date.issued | 1992 | |
| dc.identifier.citation | BOLCAL C., KOCER D., ADELMAN S., "ELEMENTAL ABUNDANCE ANALYSES WITH DAO SPECTROGRAMS .9. THE METALLIC-LINED STARS 15-VULPECULAE AND 32-AQUARII", MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.258, ss.270-276, 1992 | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.other | av_8f90cae6-c6a5-41be-bd1d-dfab50ec55b1 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/96945 | |
| dc.identifier.uri | https://doi.org/10.1093/mnras/258.2.270 | |
| dc.description.abstract | Following from previous papers of this study we present elemental abundance analyses of the sharp-lined bright Am stars 15 Vul and 32 Aqr. The values derived using fine analysis techniques are found using the stellar parameters, effective temperature and surface gravity, determined using optical-region spectrophotometry and Balmer line profiles as well as with the procedures of Moon & Dworetsky and of Lane & Lester. The latter star is a more extreme Am star than the former star. We also discuss possible ways to improve these analyses. | |
| dc.language.iso | eng | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.subject | Uzay bilimi | |
| dc.subject | Fizik | |
| dc.subject | Temel Bilimler | |
| dc.title | ELEMENTAL ABUNDANCE ANALYSES WITH DAO SPECTROGRAMS .9. THE METALLIC-LINED STARS 15-VULPECULAE AND 32-AQUARII | |
| dc.type | Makale | |
| dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 258 | |
| dc.identifier.issue | 2 | |
| dc.identifier.startpage | 270 | |
| dc.identifier.endpage | 276 | |
| dc.contributor.firstauthorID | 113746 | |
