| dc.contributor.author | MENTESE, HH | |
| dc.date.accessioned | 2021-03-03T21:02:25Z | |
| dc.date.available | 2021-03-03T21:02:25Z | |
| dc.date.issued | 1994 | |
| dc.identifier.citation | MENTESE H., "COLUMN DENSITIES OF INTERSTELLAR GAS IN THE DIRECTION OF THE STAR-EPSILON ORI-(B0-IA)", ASTROPHYSICS AND SPACE SCIENCE, cilt.220, sa.2, ss.279-287, 1994 | |
| dc.identifier.issn | 0004-640X | |
| dc.identifier.other | av_5d1f80d5-5662-4e44-87ea-90433460eff5 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/65222 | |
| dc.identifier.uri | https://doi.org/10.1007/bf00658058 | |
| dc.description.abstract | We have investigated the star epsilon Ori with IUE high resolution SWP spectrum in order to derive curve of growth and column densities of A1II, SiII, SII, FeII, NiII and ZnII. It has been possible to fit these ions on one empirical curve of growth with a velocity parameter b = 11 km s(-1) for the star studied. | |
| 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 | COLUMN DENSITIES OF INTERSTELLAR GAS IN THE DIRECTION OF THE STAR-EPSILON ORI-(B0-IA) | |
| dc.type | Makale | |
| dc.relation.journal | ASTROPHYSICS AND SPACE SCIENCE | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 220 | |
| dc.identifier.issue | 2 | |
| dc.identifier.startpage | 279 | |
| dc.identifier.endpage | 287 | |
| dc.contributor.firstauthorID | 115609 | |
