Density dependence of the line source functions in scattering media

Details Density dependence of the line source functions in scattering media Density dependence of the line source functions in scattering media

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..95..117p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 95, no. 1, Sept. 1983, p. 117-121.

Astronomy and Astrophysics

Astrophysics

Electron Density (Concentration), Electron Scattering, Radiative Transfer, Scattering Functions, Stellar Atmospheres, Line Spectra, Optical Thickness, Stellar Spectra

Scientific paper

The author has calculated source functions in a scattering medium in which the density changes according to the law of Ne(r) ≡ rn where n takes the value from -3 to +3 and Ne(r) is the electron density. He has assumed that the media consist of electrons and he has also considered a geometrically extended media in which the outer radii are 2,3,5 times the inner radius. The source functions obtained are completely due to electron scattering. It is found that the source function varies considerably for different variations of density changes from n = -3 to +3.

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