Searching evidences for spiral shocks in the quiescent accretion disk of U Gem

Details Searching evidences for spiral shocks in the quiescent accretion disk of U Gem Searching evidences for spiral shocks in the quiescent accretion disk of U Gem

2004-02-02

arxiv.org/abs/astro-ph/0402050v1

Astronomy and Astrophysics

Astrophysics

2 pages, 3 figures, to appear in RevMexAA(SC) Conference Series, Proc. of IAU Colloquium 194, Compact Binaries in the Galaxy a

Scientific paper

We find that the quiescent accretion disk of U Gem has a complicated
structure. Along to the bright spot originating in the region of interaction
between the stream and the disk particles, there are also explicit indications
of spiral shocks. The Doppler map and the variations of the peak separation of
the emission lines are indicative.

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