Parameters of the SS 433 jets - The modeling of moving-line profiles

Details Parameters of the SS 433 jets - The modeling of moving-line profiles Parameters of the SS 433 jets - The modeling of moving-line profiles

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..487b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, June 1987, p. 487-494. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astrophysics

1

Binary Stars, Gas Transport, Line Shape, Mass Transfer, Plasma Jets, Stellar Models, Emission Spectra, H Alpha Line, Nutation, Spectral Line Width

Scientific paper

The modeling of H-alpha emission line profiles in the spectra of the SS 433 jets is considered. These line profiles are compared with observed profiles obtained with the TV scanner of the 6-m telescope of the Special Astrophysical Observatory in July 1981. The main parameters of the jet are determined, including the the number of gas clouds, the H-alpha brightness profile of the jet, and the nutation angle.

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