'Transition radiation' as a possible new mechanism of emission in astrophysics

Details 'Transition radiation' as a possible new mechanism of emission in astrophysics 'Transition radiation' as a possible new mechanism of emission in astrophysics

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974poast..22..275j&link_type=abstract

Postepy Astronomii, vol. 22, Oct.-Dec. 1974, p. 275-282. In Polish.

Astronomy and Astrophysics

Astronomy

Background Radiation, Emission Spectra, Stellar Spectra, T Tauri Stars, Ultraviolet Spectra, X Ray Spectra, Compton Effect, Far Ultraviolet Radiation, Galactic Radiation, Stellar Radiation, X Ray Astronomy

Scientific paper

The physical principles of transition radiation which is generated by the steady motion of a charged particle, and takes place in the transition to a medium with different dielectric properties are outlined. The influence of this mechanism on the formation of the background radiation spectrum and the spectrum of T Tauri type stars in the ultraviolet and extreme ultraviolet is studied.

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