In this paper the integral equation (derived in Paper I) governing the fluctuations in brightness of the Milky Way is explicitly solved for the case in which the system extends to a finite distance in the direction of the line of sight and when all the clouds are equally transparent, The derived theoretical distributions are illustrated

Chandrasekhar, C.

Münch, G.

English

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The theory of the fluctuations in brightness of the Milky Way. III

http://repository.ias.ac.in/74387/1/108-p-OCR.pdf

The theory of the fluctuations in brightness of the Milky Way. III

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