Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Majlinger, Zlatko"'
Publikováno v:
In Advances in Space Research October 2024
Autor:
Almodlej, Abeer1 (AUTHOR), Majlinger, Zlatko2 (AUTHOR), Ben Nessib, Nabil1,3 (AUTHOR), Dimitrijević, Milan S.2,4 (AUTHOR) mdimitrijevic@aob.rs, Srećković, Vladimir A.5 (AUTHOR)
Publikováno v:
European Physical Journal D (EPJ D). Apr2021, Vol. 75 Issue 4, p1-5. 5p.
Usual procedure of the Stark broadening theory usage for astrophysical purpose is to determine Stark width of particular spectral line with some theoretical calculation method, and then to compare measured spectral line with synthetic line simulated
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=57a035e5b1ae::0c8f1fc0f6ec9156b36c09dea067ffa5
https://www.bib.irb.hr/1210001
https://www.bib.irb.hr/1210001
Astrophysical applications of Stark broadening theory were intensively developed in the last hundred years. For example, Verweij (1936) among the others pointed out the importance of Stark broadening influence on spectral line shapes even in the core
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::d018396b9e9cf4b1361bceb8a3d9d3ff
https://www.bib.irb.hr/1210000
https://www.bib.irb.hr/1210000
Stark Full Widths at Half Maximum for 46 Co II multiplets have been calculated in Majlinger et al. (2018) by modified semiempirical method described in Dimitrijevi{;ć}; and Konjevi{;ć}; (1980). The calculated results have been used to investigate t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::5603f43323198abf31fef1d65e106ef5
https://www.bib.irb.hr/1209929
https://www.bib.irb.hr/1209929
Data for Stark full widths at half maximum for 46 Co II multiplets were calculated using a modified semiempirical method. In order to show the applicability and usefulness of this set of data for research into white dwarf and A type star atmospheres,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::0d32da25dc9845fe27cc7be14f5f11c7
https://doi.org/10.3390/data5030074
https://doi.org/10.3390/data5030074
Simple estimates and approximations play important role in Stark broadening theory, especially in the use for astrophysical purpose. According to the statistical analysis of Stark widths obtained with modified semiempirical approach, the dependence o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=57a035e5b1ae::03e0fca9cf967c5f960f04baf715bd52
https://www.bib.irb.hr/1209923
https://www.bib.irb.hr/1209923
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Regularity and systematic trend analysis has been performed on the Stark widths of 27 Lu III spectral lines calculated elsewhere by modified semiempirical method. Possible correlation of those Stark widths with corresponding effective principal quant
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=57a035e5b1ae::005f19f8fa7af07825bc177a9c975aab
https://www.bib.irb.hr/1209921
https://www.bib.irb.hr/1209921