SS 433: The wiggle of the wind

Details SS 433: The wiggle of the wind SS 433: The wiggle of the wind

2011-07-22

arxiv.org/abs/1107.4533v2

A&A 534 A112 (2011)

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

4 pages, 3 figures. A coda to my circumbinary disk studies. To appear in A&A

Scientific paper

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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