Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Zlatko Majlinger"'
Publikováno v:
Data, Vol 5, Iss 3, p 74 (2020)
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://doaj.org/article/3eaba9e85f7248039f33d043bb7c856b
Publikováno v:
Atoms, Vol 5, Iss 4, p 49 (2017)
Regularities and systematic trends among the Stark widths of 18 Zr IV spectral lines obtained by modified semiempirical approach have been discussed. Also we compared those calculated Stark broadening parameters with estimates according to Cowley, Pu
Externí odkaz:
https://doaj.org/article/e5343730d0a348c9b5f28f900324859f
Autor:
Zlatko Majlinger, Nabil Ben Nessib, Vladimir A. Srećković, Milan S. Dimitrijević, Abeer Al-Modlej
Publikováno v:
The European Physical Journal D : Atomic, molecular, optical and plasma physics
The European Physical Journal D : Atomic, molecular, optical and plasma physics, EDP Sciences, 2021, 75 (4), pp.141. ⟨10.1140/epjd/s10053-021-00149-w⟩
The European Physical Journal D : Atomic, molecular, optical and plasma physics, EDP Sciences, 2021, 75 (4), pp.141. ⟨10.1140/epjd/s10053-021-00149-w⟩
The neglecting of Stark broadening in analysis and synthesis of hot stars spectra in some cases could cause errors in abundance determination. We analysed Co II lines in the spectrum of $$\chi $$ Lupi and found two well-isolated and strong lines ( $$
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0dba43fde3eff0a26115b3498932450
https://hal.archives-ouvertes.fr/hal-03508637
https://hal.archives-ouvertes.fr/hal-03508637
Publikováno v:
Data, Vol 5, Iss 74, p 74 (2020)
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,
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=doi_dedup___::dd59217d71f590b0612117cabe0a2927
https://www.bib.irb.hr/1209918
https://www.bib.irb.hr/1209918
Stark full widths at half-maximum for 46 Co ii multiplets have been calculated using modified semi-empirical method. The obtained results have been used to demonstrate the importance of Stark broadening mechanism in DA and DB white dwarf and A star a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a41f71eacce59604981a96661f1b23fe
https://doi.org/10.1093/mnras/staa1947
https://doi.org/10.1093/mnras/staa1947
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 470 (2), pp.1911-1918. ⟨10.1093/mnras/stx1321⟩
Monthly Notices of the Royal Astronomical Society, 2017, 470 (2), pp.1911-1918. ⟨10.1093/mnras/stx1321⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 470 (2), pp.1911-1918. ⟨10.1093/mnras/stx1321⟩
Monthly Notices of the Royal Astronomical Society, 2017, 470 (2), pp.1911-1918. ⟨10.1093/mnras/stx1321⟩
Stark widths for 18 Zr IV spectral lines have been calculated by using the modified semi-empirical method. The obtained results have been used to investigate the influence of Stark broadening on the spectra of atmospheres of chemically peculiar stars
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::512330b930ba75f98dd42fd03ea96003
https://hal.archives-ouvertes.fr/hal-02240914
https://hal.archives-ouvertes.fr/hal-02240914
Publikováno v:
Journal of Astrophysics and Astronomy
Journal of Astrophysics and Astronomy, Indian Academy of Sciences, 2015, 36 (4), ⟨10.1007/s12036-015-9362-9⟩
Journal of Astrophysics and Astronomy, 2015, 36 (4), ⟨10.1007/s12036-015-9362-9⟩
Journal of Astrophysics and Astronomy, Indian Academy of Sciences, 2015, 36 (4), ⟨10.1007/s12036-015-9362-9⟩
Journal of Astrophysics and Astronomy, 2015, 36 (4), ⟨10.1007/s12036-015-9362-9⟩
The electron-impact widths for 27 Lu III spectral lines have been calculated by using the modified semiempirical method. Calculations have been also performed with the published relativistic Hartree-Fock oscillator strengths and additionally, with th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2ae5e598ff1f4ba1114a5261490616ff
https://hal.archives-ouvertes.fr/hal-02397893
https://hal.archives-ouvertes.fr/hal-02397893