| dc.contributor.author | GUZEL, T | |
| dc.contributor.author | BOLCAL, C | |
| dc.contributor.author | KOCER, D | |
| dc.contributor.author | KOKTAY, T | |
| dc.date.accessioned | 2021-03-04T10:41:24Z | |
| dc.date.available | 2021-03-04T10:41:24Z | |
| dc.date.issued | 1991 | |
| dc.identifier.citation | BOLCAL C., KOCER D., KOKTAY T., GUZEL T., "A MODEL-ATMOSPHERE ANALYSIS OF AP STAR HD 26385", ASTROPHYSICS AND SPACE SCIENCE, cilt.185, sa.2, ss.237-247, 1991 | |
| dc.identifier.issn | 0004-640X | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.other | av_6e77785b-a098-4ab7-9b26-5aa126eaaaa7 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/76267 | |
| dc.identifier.uri | https://doi.org/10.1007/bf00643191 | |
| dc.description.abstract | An abundance analysis using photographic region spectrograms and fully line-blanketed model atmospheres has been performed for the chemically peculiar (CP) star HD 26385. Model parameters were determined from H-gamma-profile and photometric data. Its pattern of abundance shows that HD 26385 is typically Ap Si-star. | |
| dc.language.iso | eng | |
| dc.subject | Uzay bilimi | |
| dc.subject | ASTRONOMİ VE ASTROFİZİK | |
| dc.subject | Temel Bilimler (SCI) | |
| dc.subject | Fizik | |
| dc.subject | Astronomi ve Astrofizik | |
| dc.subject | Temel Bilimler | |
| dc.title | A MODEL-ATMOSPHERE ANALYSIS OF AP STAR HD 26385 | |
| dc.type | Makale | |
| dc.relation.journal | ASTROPHYSICS AND SPACE SCIENCE | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 185 | |
| dc.identifier.issue | 2 | |
| dc.identifier.startpage | 237 | |
| dc.identifier.endpage | 247 | |
| dc.contributor.firstauthorID | 113130 | |
