The authors discuss the implications of the 6.7 keV line detection on the jet model for SS433. In particular, they constrain the physical parameters, i.e. density and temperature, of the jets and re-examine the thermal instability mechanism proposed for the jet fragmentation.

On the X-ray emission from SS433

FERRARI, Attilio;MASSAGLIA, Silvano;
1988-01-01

Abstract

The authors discuss the implications of the 6.7 keV line detection on the jet model for SS433. In particular, they constrain the physical parameters, i.e. density and temperature, of the jets and re-examine the thermal instability mechanism proposed for the jet fragmentation.
1988
27
5
11
Bodo, G.; Ferrari, A.; Massaglia, S.; Brinkmann, W.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/110558
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