Color temperatures of objects with electron scattering

Details Color temperatures of objects with electron scattering Color temperatures of objects with electron scattering

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980afz....16..695s&link_type=abstract

(Astrofizika, vol. 16, Oct.-Dec. 1980, p. 695-706.) Astrophysics, vol. 16, no. 4, Apr. 1981, p. 400-407. Translation.

Astronomy and Astrophysics

Astrophysics

9

Electron Scattering, Photosphere, Stellar Radiation, Stellar Spectrophotometry, Absorptivity, Atmospheric Models, Integral Equations, Optical Thickness

Scientific paper

The radiation flux that emerges from a stellar photosphere when the coefficient of electron scattering has a constant ratio to the coefficient of true absorption is determined. The problem is solved by exact and approximate methods. The spectrophotometric gradient is determined as a function of the parameters characterizing the photosphere; and it is shown that the electron scattering can both raise and lower the color temperature. Electron scattering in photospheres of WR stars is considered as an example.

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