Inverse Compton effect and the colorimetric characteristics of flare stars

Details Inverse Compton effect and the colorimetric characteristics of flare stars Inverse Compton effect and the colorimetric characteristics of flare stars

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..80..211g&link_type=abstract

Astrophysics and Space Science, vol. 80, no. 1, Nov. 1981, p. 211-230.

Astronomy and Astrophysics

Astronomy

Compton Effect, Flare Stars, Hertzsprung-Russell Diagram, Inverse Scattering, Photon-Electron Interaction, Stellar Radiation, Ultraviolet Spectra, Indexes (Ratios), Infrared Astronomy, Photosphere, Radiation Distribution, Stellar Models

Scientific paper

It is shown that observed color diagrams for pure flare emission of UV Cet type flare stars may be explained within the framework of a fast electron hypothesis. The pronounced influence on these color indices of the following two factors is shown: (1) the deviations of the normal radiation capability of the star in the infrared region from the Planckian distribution and (2) the location of the cloud (source) of fast electrons around the star (flare 'geometry effect'). The possible role of a reflection effect at the generation of stellar flares is discussed.

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