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SS 433 as a Magnetic X-Ray Binary

Published online by Cambridge University Press:  14 August 2015

G.W. Collins II ,
G. H. Newsom  and
R. N. Boyd
G.W. Collins II
Affiliation:
The Ohio State University
G. H. Newsom
Affiliation:
The Ohio State University
R. N. Boyd
Affiliation:
The Ohio State University

Abstract

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In this paper we expand upon a proposed model for SS 433. Specific attention is given to the manner in which the light travel time within the system places constraints upon the geometrical parameters defining the system. Consideration is also given to the physical situation which exists in the high Doppler shift emitting region. Implications of recent observations of “a 13-day” period spectral and light variability upon the central source are briefly discussed.

Type
VI. X-Ray Binaries
Information
Symposium - International Astronomical Union , Volume 88: Close Binary Stars: Observations and Interpretation , 1980 , pp. 375 - 379
Copyright
Copyright © Reidel 1980 

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