Redistribution effects on line formation in moving stellar atmospheres—I. The isotropic redistribution function RI−A(x′, x; v)
- 1 September 1974
- journal article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 14 (9) , 909-918
- https://doi.org/10.1016/0022-4073(74)90018-1
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Redshifted Line Profiles from Differentially Expanding AtmospheresThe Astrophysical Journal, 1968
- Line formation in a differentially moving non-lte atmosphereJournal of Quantitative Spectroscopy and Radiative Transfer, 1968
- Improved Boundary Conditions for the Feautrier MethodThe Astrophysical Journal, 1967
- The Velocity-Dependent Non-Lte Source Function. I. Discontinuous Velocity-Semi AtmosphereThe Astrophysical Journal, 1967
- Thermalization Lengths and the Homogeneous Transfer Equation in Line FormationThe Astrophysical Journal, 1966
- Non-LTE line formation with spatial variations in the Doppler widthJournal of Quantitative Spectroscopy and Radiative Transfer, 1966
- Emission and absorption profiles in a scattering atmosphereJournal of Quantitative Spectroscopy and Radiative Transfer, 1965
- Radiative transfer of Doppler broadened resonance lines: IIProceedings of the Physical Society, 1964
- Non-Coherent Scattering: I. The Redistribution Function with Doppler BroadeningMonthly Notices of the Royal Astronomical Society, 1962
- The Source Function in a Non-Equilibrium Atmosphere. I. The Resonance Lines.The Astrophysical Journal, 1957