Structure of the pre-outburst accretion disk in SS Cygni

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Fig. 6

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Doppler tomograms in the H_β line. The upper panel is computed using the data of August 2006, while the lower panel is computed using the new data. Markers are the same as in Figs. 2 and 5. Certain isolines are plotted to select regions of tidal shock (lower left quadrants of the tomograms).

This figure is made of several images, please see below:

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Open with DEXTER

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