X ray observations of SS433 and its jets

Details X ray observations of SS433 and its jets X ray observations of SS433 and its jets

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..163s&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 163-170 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

4

Emission Spectra, Stellar Mass Ejection, Stellar Orbits, Stellar Spectra, X Ray Spectra, Compton Effect, Exosat Satellite, Japanese Space Program, Precession, Spectrum Analysis, Stellar Mass, Stellar Structure

Scientific paper

The EXOSAT and Ginga observations of SS433 are discussed. They are used to show that the major factors in determining the variations in the X-ray emission from the jets of SS433 are precessional and orbital geometric influences. Limits on the sizes and masses of the system components and the structure of the X-ray emitting material within the jets are derived. Evidence that the line profile is significantly variable with precession phase suggest that some Compton broadening of the line is required.

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