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Possible origin of the radio emission from SS433 jets

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Abstract

It is shown that radio emission from the jet of the galactic source SS433 as well as the variability of its flux density could be accounted for by the inelastic collision model. Variability in the jet flux is attributed mainly to the variability in the thermal proton number density available in the jet regions.

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Authors and Affiliations

  1. Astrophysics Research Group, Department of Physics and Astronomy, University of Nigeria, Nsukka, Nigeria

    S. S. Nweze, P. N. Okeke & M. W. Anyakoha

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  1. S. S. Nweze
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  2. P. N. Okeke
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  3. M. W. Anyakoha
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Nweze, S.S., Okeke, P.N. & Anyakoha, M.W. Possible origin of the radio emission from SS433 jets. Astrophys Space Sci 173, 257–263 (1990). https://doi.org/10.1007/BF00643935

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  • DOI: https://doi.org/10.1007/BF00643935

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