Results 1 to 10 of about 92,545 (152)
Stark Broadening and White Dwarfs [PDF]
Open Astronomy, 2011 White dwarf and pre-white dwarfs are the best types of stars for the application of Stark broadening research results in astrophysics, since in the atmospheres of these stars physical conditions are very favorable for this line broadening mechanism - in ...
Dimitrijević Milan S. +3 more
doaj +4 more sources
Stark Broadening of Several Ne II, Ne III and O III Spectral Lines for the Stark-B Database [PDF]
Open Astronomy, 2011 In order to complete Stark broadening data for Ne II and O III lines, needed for analysis of stellar atmospheres, we determined the missing parameters for the broadening by collisions with protons and ionized helium for 15 Ne II and 5 O III multiplets ...
Dimitrijević Milan S. +3 more
doaj +5 more sources
Data, 2020 The aim of this paper is to analyze the various uses of Stark broadening data for non-hydrogenic lines emitted from plasma, obtained with the modified semiempirical method formulated 40 years ago (1980), which are continuously implemented in the STARK-B ...
Milan S Dimitrijevic
exaly +3 more sources
On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation Approach
Atoms, 2014 The significance of Stark broadening data for problems in astrophysics, physics, as well as for technological plasmas is discussed and applications of Stark broadening parameters calculated using a semiclassical perturbation method are analyzed.
Milan S Dimitrijevic +1 more
exaly +3 more sources
Stark Broadening of Several Ar I Spectral Lines in the Visible Spectrum
Open Astronomy, 2011 In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we determined Stark widths and shifts due to electron, proton and ionized helium impacts for nine lines (4191.0, 4259.4, 5912.1, 6043.2, 6045.0, 6752.9, 7503 ...
Dimitrijević Milan S. +3 more
doaj +5 more sources
Stark Broadening of In III Lines in Astrophysical and Laboratory Plasma
Open Astronomy, 2011 In the deeper layers of hot stellar photospheres the Stark widths of spectral lines can be comparable and even larger than the thermal Doppler widths.
Simić Z. +3 more
doaj +3 more sources
Stark Broadening of Co II Lines in Stellar Atmospheres
Data, 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, the
Milan S Dimitrijevic +1 more
exaly +3 more sources
Stark Broadening of Se IV, Sn IV, Sb IV and Te IV Spectral Lines
Atoms, 2018 Stark broadening parameters, line width and shift, are needed for investigations, analysis and modelling of astrophysical, laboratory, laser produced and technological plasmas.
Milan S Dimitrijevic +2 more
exaly +3 more sources
Stark Broadening of Cr III Spectral Lines: DO White Dwarfs
Atoms, 2018 Using the modified semiempirical method of Dimitrijević and Konjević, Stark widths have been calculated for six Cr III transitions, for an electron density of 10 17 cm ‒ 3 and for temperatures from 5000–80,000 K.
Milan S Dimitrijevic
exaly +3 more sources
Atoms, 2021 Analysis of Stark-broadened spectral line profiles is a powerful, non-intrusive diagnostic technique to extract the electron density of high-energy-density plasmas. The increasing number of applications and availability of spectroscopic measurements have
Marco A. Gigosos +3 more
doaj +1 more source