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

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dc.creatorNeustroev, V. V.
dc.creatorChavushyan, V.
dc.creatorValdes, J. R.
dc.date2004-02-02
dc.date.accessioned2026-07-07T02:12:05Z
dc.date.available2026-07-07T02:12:05Z
dc.descriptionWe 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.
dc.description2 pages, 3 figures, to appear in RevMexAA(SC) Conference Series, Proc. of IAU Colloquium 194, Compact Binaries in the Galaxy and Beyond, La Paz, Mexico, 17-21 Nov., 2003
dc.identifierhttps://arxiv.org/abs/astro-ph/0402050
dc.identifierhttp://arxiv.org/abs/astro-ph/0402050
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7337
dc.subjectAstrophysics
dc.titleSearching evidences for spiral shocks in the quiescent accretion disk of U Gem
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