The relativistic Doppler-broadened profile of an absorption line due to the thermal motion of light-absorbing particles is formulated. The obtained profile of an absorption line is asymmetrically broadened with more weight in the redshift wing than in the blueshift wing. Moreover, the peak frequency of the profile of an absorption line evinces red-shifting with increasing temperature
Analytical expressions for total radiances and equivalent widths of isolated spectral lines with com...
Compton energy absorption cross sections are calculated using the formulas based on a relativistic...
ABSTRACT: In this paper, we derived more general and correct expressions for the Relativistic Doppl...
The relativistic Doppler broadening of the line emission from both thermal and power-law particle di...
In this work, we report some relativistic effects on the spectral line broadening. In particular, we...
peer reviewedThe probabilistic approach of Surdej (1979) is followed to generalize the Sobolev (1958...
The Doppler parameter distribution of Lyman-alpha absorption is calculated for a set of different re...
Author Institution: Obukhov Institute of Atmospheric Physics, Siberian Branch, Russian Academy of Sc...
The Doppler parameter distribution of Ly#alpha# absorption is calculated for a set of different reio...
All bodies in the universe are constantly absorbing heat from surrounding thermal sources. This heat...
Methods are described for calculating the spectral absorption coefficient for lines with combined Do...
The emission line profile of an atom in a dissipative medium is investigated theoretically by Langev...
An analytical method similar to that used by (1) on Lorentz lines was applied to the problem of the ...
We investigate the influence of dispersion and relativistic effects on the spectral line-shape model...
Spectral line formation is examined in simple model atmospheres when there are deviations from compl...
Analytical expressions for total radiances and equivalent widths of isolated spectral lines with com...
Compton energy absorption cross sections are calculated using the formulas based on a relativistic...
ABSTRACT: In this paper, we derived more general and correct expressions for the Relativistic Doppl...
The relativistic Doppler broadening of the line emission from both thermal and power-law particle di...
In this work, we report some relativistic effects on the spectral line broadening. In particular, we...
peer reviewedThe probabilistic approach of Surdej (1979) is followed to generalize the Sobolev (1958...
The Doppler parameter distribution of Lyman-alpha absorption is calculated for a set of different re...
Author Institution: Obukhov Institute of Atmospheric Physics, Siberian Branch, Russian Academy of Sc...
The Doppler parameter distribution of Ly#alpha# absorption is calculated for a set of different reio...
All bodies in the universe are constantly absorbing heat from surrounding thermal sources. This heat...
Methods are described for calculating the spectral absorption coefficient for lines with combined Do...
The emission line profile of an atom in a dissipative medium is investigated theoretically by Langev...
An analytical method similar to that used by (1) on Lorentz lines was applied to the problem of the ...
We investigate the influence of dispersion and relativistic effects on the spectral line-shape model...
Spectral line formation is examined in simple model atmospheres when there are deviations from compl...
Analytical expressions for total radiances and equivalent widths of isolated spectral lines with com...
Compton energy absorption cross sections are calculated using the formulas based on a relativistic...
ABSTRACT: In this paper, we derived more general and correct expressions for the Relativistic Doppl...