| dc.contributor.author | Cay, IH | |
| dc.contributor.author | Tektunali, HG | |
| dc.contributor.author | Adelman, SJ | |
| dc.contributor.author | Caliskan, H | |
| dc.contributor.author | Kocer, D | |
| dc.date.accessioned | 2021-03-06T10:30:18Z | |
| dc.date.available | 2021-03-06T10:30:18Z | |
| dc.date.issued | 2000 | |
| dc.identifier.citation | Adelman S., Caliskan H., Kocer D., Cay I., Tektunali H., "Elemental abundance analyses with DAO spectrograms - XXIII. The superficially normal stars 28 And (A7 III) and 99 Her (F7 V)", MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.316, ss.514-518, 2000 | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.other | av_eaade76d-7989-448a-9fd5-79d46abfd840 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/154143 | |
| dc.identifier.uri | https://doi.org/10.1046/j.1365-8711.2000.03577.x | |
| dc.description.abstract | Elemental abundances of 28 And (A7 III) and 99 Her (F7 V), which have modest rotational velocities, are derived in a manner consistent with previous studies in this series of papers. The values for 28 And, a delta Scuti variable, show that it is slightly metal-poor, but not a classical Am star. 99 Her, which is somewhat more metal-poor, has a rather small microturbulence for its spectral type. | |
| 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 - XXIII. The superficially normal stars 28 And (A7 III) and 99 Her (F7 V) | |
| dc.type | Makale | |
| dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 316 | |
| dc.identifier.issue | 3 | |
| dc.identifier.startpage | 514 | |
| dc.identifier.endpage | 518 | |
| dc.contributor.firstauthorID | 126265 | |
