On the ratio of the X-ray and gamma-ray emission of SS 443

Details On the ratio of the X-ray and gamma-ray emission of SS 443 On the ratio of the X-ray and gamma-ray emission of SS 443

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..903b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Dec. 1984, p. 903-907) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Nov.-Dec

Physics

Nuclear Physics

Binary Stars, Gamma Ray Astronomy, Variable Stars, X Ray Astronomy, Electron Scattering, Elementary Particle Interactions, Interstellar Gas, Luminosity, Nuclei (Nuclear Physics), Plasma Jets, Spectral Line Width

Scientific paper

The ratio of the fluxes of X-ray emission generated by heavy particles in the interaction with ambient electrons and of γ-ray line emission generated by the same particles is obtained. A probable model of interaction of the matter ejected from SS433 with its environment is distinguished from comparison of the calculations with observations of the SS433 object. The abundance of nuclei emitting γ-quanta in the ejected matter is obtained to be no less than 1/50 with respect to hydrogen.

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