Kepler tomography of the accretion disk in V436 Centauri

Details Kepler tomography of the accretion disk in V436 Centauri Kepler tomography of the accretion disk in V436 Centauri

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..485h&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

Scientific paper

We present preliminary results from a Doppler tomographic study of the accretion disk in the SU UMa dwarf nova V436 Cen. We have constructed tomograms in the rotating frames of many different individual accretion disk annulae: Kepler tomography. This technique -- the equivalent of a 3-dimensional periodogram (Vx, Vy, Ptomo) -- can be used to look for traces of structures -- like waves, magnetic prominences and loops within the disk.

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