| dc.contributor.author | MENTESE, HH | |
| dc.date.accessioned | 2021-03-03T10:50:30Z | |
| dc.date.available | 2021-03-03T10:50:30Z | |
| dc.date.issued | 1992 | |
| dc.identifier.citation | MENTESE H., "RELATION BETWEEN ELEMENT DEPLETION AND INTERSTELLAR REDDENING IN THE DIRECTION OF OB STARS", ASTROPHYSICS AND SPACE SCIENCE, cilt.187, sa.1, ss.127-133, 1992 | |
| dc.identifier.issn | 0004-640X | |
| dc.identifier.other | av_24e3e82d-c672-4def-9410-ee04d9275df4 | |
| dc.identifier.other | vv_1032021 | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12627/29683 | |
| dc.identifier.uri | https://doi.org/10.1007/bf00642693 | |
| dc.description.abstract | We have studied the interstellar column densities of AlII, SiII, SII, FeII, NiII, and ZnII in the direction of 18 O- and 6 B-type stars so as to improve the relations of element depletions with E(B-V), and to look for other possible relations with two stellar parameters: namely, the rate of mass loss and rotational velocity. The stars were chosen in order to cover several directions in the Galaxy, as well as a wide range in interstellar reddening. We found a clear inverse trend relating the abundance of elements to interstellar reddening. | |
| 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 | RELATION BETWEEN ELEMENT DEPLETION AND INTERSTELLAR REDDENING IN THE DIRECTION OF OB STARS | |
| dc.type | Makale | |
| dc.relation.journal | ASTROPHYSICS AND SPACE SCIENCE | |
| dc.contributor.department | , , | |
| dc.identifier.volume | 187 | |
| dc.identifier.issue | 1 | |
| dc.identifier.startpage | 127 | |
| dc.identifier.endpage | 133 | |
| dc.contributor.firstauthorID | 113172 | |
