The Effect of Strong Scattering Processes in the Continuum on the Stellar Emergent Energy Distribution
The numerical solution of the idealized, but self-consistent, LTE atmosphere problem posed by the authors has been used to introduce the effect of multiple scattering on the temperature gradient, the spectral distribution of the observed flux and the intensity discontinuities. In the theoretical consideration of the problem, the nature of
Nikoghossian, A. et al.
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1996