| dc.contributor.author | Caliskan, Hülya | |
| dc.contributor.author | ADELMAN, SJ | |
| dc.date.accessioned | 2021-03-02T23:02:52Z | |
| dc.date.available | 2021-03-02T23:02:52Z | |
| dc.date.issued | 1997 | |
| dc.identifier.citation | Caliskan H., ADELMAN S., "Elemental abundance analyses with DAO spectrograms .17. The superficially normal early A stars 2 Lyncis, omega Ursa Majoris and phi Aquilae", MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.288, sa.2, ss.501-511, 1997 | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_10286765-58c8-45ec-a301-79943c3d85db | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/16383 | |
| dc.identifier.uri | https://doi.org/10.1093/mnras/288.2.501 | |
| dc.description.abstract | Elemental abundances of the superficially normal early A stars 2 Lyn, omega UMa and phi Aql are derived consistent with previous studies in this series, using spectrograms obtained with Reticon and CCD detectors. The derived elemental abundances of 2 Lyn are usually very close to solar. Both omega UMa and phi Aql, which are considered to be hot metallic-line stars, show He underabundances as well as overabundances of many iron-peak and heavier elements. | |
| dc.language.iso | eng | |
| dc.subject | Uzay bilimi | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.subject | Fizik | |
| dc.subject | Temel Bilimler | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.title | Elemental abundance analyses with DAO spectrograms .17. The superficially normal early A stars 2 Lyncis, omega Ursa Majoris and phi Aquilae | |
| dc.type | Makale | |
| dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 288 | |
| dc.identifier.issue | 2 | |
| dc.identifier.startpage | 501 | |
| dc.identifier.endpage | 511 | |
| dc.contributor.firstauthorID | 51640 | |
