Please use this identifier to cite or link to this item:
https://research.matf.bg.ac.rs/handle/123456789/973| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Dimitrijević, Milan S. | en_US |
| dc.contributor.author | Kovačević, Anđelka | en_US |
| dc.contributor.author | Simić, Zoran | en_US |
| dc.contributor.author | Sahal-Bréchot, Sylvie | en_US |
| dc.date.accessioned | 2022-08-16T11:22:38Z | - |
| dc.date.available | 2022-08-16T11:22:38Z | - |
| dc.date.issued | 2010-01-01 | - |
| dc.identifier.isbn | 9781632662194 | - |
| dc.identifier.uri | https://research.matf.bg.ac.rs/handle/123456789/973 | - |
| dc.description.abstract | In order to provide Stark broadening data in X-ray and far UV wavelength region, of interest for modelling and analysis of astrophysical plasmas in extreme conditions, we performed calculations of Stark broadened line widths and shifts for Ar XV using the semiclassical perturbation theory. | en |
| dc.relation.ispartof | Publikacije astronomskog društva "Rudjer Bošković" | en_US |
| dc.title | On the stark broadening of Ar XV spectral lines | en_US |
| dc.type | Conference Paper | en_US |
| dc.relation.publication | VII Serbian-Bulgarian Astronomical Conference, SBAC 2010 | en_US |
| dc.identifier.scopus | 2-s2.0-84902449072 | - |
| dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/84902449072 | - |
| dc.contributor.affiliation | Astronomy | en_US |
| dc.relation.firstpage | 243 | en_US |
| dc.relation.lastpage | 246 | en_US |
| dc.relation.volume | 11 | en_US |
| item.fulltext | No Fulltext | - |
| item.openairetype | Conference Paper | - |
| item.grantfulltext | none | - |
| item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
| item.cerifentitytype | Publications | - |
| crisitem.author.dept | Astronomy | - |
| crisitem.author.orcid | 0000-0001-5139-1978 | - |
| Appears in Collections: | Research outputs | |
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