Приказ основних података о документу
On the Stark broadening of the Re II spectral lines
dc.creator | Simić, Zoran | |
dc.creator | Milovanović, Nenad | |
dc.creator | Sakan, Nenad | |
dc.creator | Malović, Miodrag | |
dc.date.accessioned | 2023-01-13T10:22:57Z | |
dc.date.available | 2023-01-13T10:22:57Z | |
dc.date.issued | 2023 | |
dc.identifier.issn | 0273-1177 | |
dc.identifier.uri | http://TechnoRep.tmf.bg.ac.rs/handle/123456789/5351 | |
dc.description.abstract | Stark broadening parameters - full widths at half maximum (FWHM) and shifts for 11 Re II lines have been calculated. The plasma parameters used were electron density of 1017 cm−3 and temperature from 5 000 K to 80 000 K. Calculations were performed using the simplified modified semiempirical (SMSE) approach and compared with calculations by Cowley’s approximative Stark broadening formula at 10000 K, usefull in spectrum synthesis. The results have also been considered in the atmosphere model of A type star and for DB white dwarfs. | sr |
dc.language.iso | en | sr |
dc.publisher | Elsevier Ltd. | sr |
dc.relation | info:eu-repo/grantAgreement/MESTD/inst-2020/200002/RS// | sr |
dc.relation | info:eu-repo/grantAgreement/MESTD/inst-2020/200287/RS// | sr |
dc.rights | restrictedAccess | sr |
dc.source | Advances in Space Research | sr |
dc.subject | Stark broadening | sr |
dc.subject | Spectral lines | sr |
dc.subject | Line profiles | sr |
dc.title | On the Stark broadening of the Re II spectral lines | sr |
dc.type | article | sr |
dc.rights.license | ARR | sr |
dc.citation.epage | 1292 | |
dc.citation.issue | 2 | |
dc.citation.rank | M21~ | |
dc.citation.spage | 1287 | |
dc.citation.volume | 71 | |
dc.identifier.doi | 10.1016/j.asr.2022.07.079 | |
dc.identifier.scopus | 2-s2.0-85136466166 | |
dc.type.version | publishedVersion | sr |