Photometric study of eclipsing dwarf nova EX Dra
February 25, 2021
We have analyzed long-term photometric observations of the dwarf nova EX Dra, a system with a long orbital period, in quiescence, the pre-outburst state, and the active state. The aim of our study was to test the hypothesis of Baptista  that the outbursts in this system are due to an increasing rate of mass outflow from the secondary rather than the thermal instability associated with changing viscosity in the disk
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