SS433 - The puzzle continues

Details SS433 - The puzzle continues SS433 - The puzzle continues

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...218l..13b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 218, no. 1-2, July 1989, p. L13-L16.

Astronomy and Astrophysics

Astronomy

27

Black Holes (Astronomy), Neutron Stars, X Ray Binaries, Light Curve, Roche Limit, Supernova Remnants

Scientific paper

Two recent observations of SS433 with the X-ray astronomy satellite Ginga, centered at the phases of optical primary minimum revealed new information about the systems binary properties. However, the X-ray and optical data seem to be inconsistent with the standard interpretation of a primary, filling its Roche lobe. Therefore, the question of the nature of the compact object, a neutron star or a black hole, remains open. The analysis of the X-ray data indicates that the precessing jets are rotating retrograde with respect to the orbital binary motion.

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