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astro-ph.GA2011★ 6 cited
SS 433: The wiggle of the wind
M. G. Bowler
The Balmer H alpha emission line in the stationary spectrum of SS 433 has a component originating in the wind above the accretion disk. The Doppler motion of this line is a blurred…
astro-ph.GA2011
On Purple Mountain Halpha observations of SS 433
M G Bowler
In this brief note I draw attention to the structure of the stationary Halpha line as a function of orbital phase, using a data set compiled over some years. These data are compare…