On the X-ray emission from SS433

Details On the X-ray emission from SS433 On the X-ray emission from SS433

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apl%26c..27....5b&link_type=abstract

Astrophysical Letters and Communications (ISSN 0888-6512), vol. 27, June 1988, p. 5-11.

Astronomy and Astrophysics

Astronomy

2

Astronomical Models, Plasma Jets, Radio Jets (Astronomy), Relativistic Plasmas, X Ray Sources, Accretion Disks, Black Holes (Astronomy), Doppler Effect, Kinetic Energy, Line Spectra, Thermal Instability

Scientific paper

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.

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