Constraints on the SS433 system from the GINGA observations

Details Constraints on the SS433 system from the GINGA observations Constraints on the SS433 system from the GINGA observations

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..701z&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 701-703 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

1

Black Holes (Astronomy), Eclipsing Binary Stars, Ginga Satellite, Japanese Space Program, Satellite Observation, Stellar Models, X Ray Binaries, Stellar Mass, Stellar Mass Ejection, Stellar Occultation, Stellar Orbits, Time Measurement

Scientific paper

Recent X ray observations with the Ginga satellite of the X ray eclipse in the binary system SS433 are examined. They confirmed and implemented the previous observations with the EXOSAT satellite. The assumptions that allow proceeding from observed data to estimates of the mass of the compact object and the size of the jets are investigated. The results are used to constrain the mass of the compact object in order to clarify its nature. The question concerning the mechanism for the possible transition from a quiescent to an active X ray phase of the system and the connection of exact timing of the X ray eclipses with the sense of the orbital motion are investigated.

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