Possible origin of the radio emission from SS433 jets

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...

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Veröffentlicht in:	Astrophysics and space science 1990-11, Vol.173 (2), p.257-263
Hauptverfasser:	NWEZE, S. S, OKEKE, P. N, ANYAKOHA, M. W
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology Stellar systems. Galactic and extragalactic objects and systems. The universe Unidentified sources and radiation outside the solar system X-ray sources x-ray bursts
Online-Zugang:	Volltext
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Zusammenfassung:	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. (Author)
ISSN:	0004-640X 1572-946X
DOI:	10.1007/BF00643935