Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..663f&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Aug. 1987, p. 663-670. In Russian. In Russian. In Russian.
Astronomy and Astrophysics
Astronomy
H Alpha Line, Mass Distribution, Plasma Jets, Spectrum Analysis, Spiral Galaxies, Interstellar Extinction, Kinetic Energy
Scientific paper
Mass loss rate in the SS433 jets is estimated to be Mj ≈ 5×10-7M_sun;/y. The parameters of the Hα clouds in the jet: dimensions and density, filling factor are presented. Gas in the clouds is heated by the hard radiation of the disk with ɛ ≥ 0.5 keV. This radiation should be strongly collimated along the jets, the opening angle of the radiation cone is θc < 13°. Arguments for θc ≈ 6° are presented. The possible radiation cone structure is discussed.
Borisov N. V.
Fabrika Sergei N.
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