Ag. Nikoghossian et Gl. Israelian, THE EFFECT OF STRONG SCATTERING PROCESSES IN THE CONTINUUM ON THE STELLAR EMERGENT ENERGY-DISTRIBUTION, Journal of quantitative spectroscopy & radiative transfer, 56(4), 1996, pp. 501-507
The numerical solution of the idealized, but self-consistent, LTE atmo
sphere problem posed by the authors has been used to introduce the eff
ect of multiple scattering on the temperature gradient, the spectral d
istribution of the observed flux and the intensity discontinuities. In
the theoretical consideration of the problem, the nature of scatterin
g processes is not concretized because, in general, common Thomson sca
ttering on free electrons is not necessarily the only nor the most eff
ective mechanism among the scattering processes. Copyright (C) 1966 El
sevier Science Ltd