TL;DR
This paper explains the Doppler motion of the Balmer H alpha emission line in SS 433 as a result of wind emission above the accretion disk, lasting several days and reflecting the motion of the compact object.
Contribution
It introduces a model linking the wind emission's Doppler motion to the accreting compact object's movement, providing insight into the emission's temporal behavior.
Findings
The H alpha emission component originates in the wind above the accretion disk.
Emission lasts over a few days, similar to jet bolide radiation.
Doppler motion reflects the compact object's movement.
Abstract
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 representation of the motion of the compact object accreting. I show how this may be understood in terms of emission lasting over a few days, like radiation from the jet bolides.
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