Line Formation in Turbulent Media
- 1 January 1975
- book chapter
- Published by Springer Nature
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- The velocity-dependent source function in radiative transfer theoryJournal of Quantitative Spectroscopy and Radiative Transfer, 1974
- Analyses of light-ion spectra in stellar atmospheres.V. Neon I in B stars.The Astrophysical Journal, 1973
- Analyses of Light Ion Spectra in Stellar Atmospheres.IV. H II in the B StarsThe Astrophysical Journal Supplement Series, 1973
- A non-LTE study of silicon line formation in early-type main-sequence atmospheres.The Astrophysical Journal, 1973
- Analyses of Light-Ion Spectra in Stellar Atmospheres. I. Magnesium II in B and O StarsThe Astrophysical Journal, 1972
- Redshifted Line Profiles from Differentially Expanding AtmospheresThe Astrophysical Journal, 1968
- Solution of Radiative Transfer Problems Using the Invariant Sn MethodMonthly Notices of the Royal Astronomical Society, 1968
- Theoretical Line Intensities.VI. Milne-Eddington Curves of Growth for Non-Coherent ScatteringThe Astrophysical Journal, 1968
- Line formation in a differentially moving non-lte atmosphereJournal of Quantitative Spectroscopy and Radiative Transfer, 1968
- Stochastic Problems in Physics and AstronomyReviews of Modern Physics, 1943