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On the Problem of Transfer of Radiation in a Spherically Symmetrical Stellar Atmosphere for the Non-Conservative Case
On the Problem of Softening of Radiation by Multiple Compton Scattering in Stellar Atmospheres containing Free-Electrons
An Estimate of the Optical Thickness of a Spherically Symmetric, Non-conservative Scattering Atmosphere
Trigonometrical Series Method in Solving the Problem of Softening and Degree of Polarization of Radiation in an Electron Atmosphere, scattering according to Rayleigh' Law and Involving Compton Change in Wavelength
Method of Trigonometrical Series in Calculating the Modification of Intensity of Monochromatic Radiation due to Multiple Compton Scattering in Stellar Atmosphere