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Outbursts in two classes of interacting binary systems, the symbiotic stars(SSs) and the cataclysmic variables (CVs), show a number of similarities inspite of very different orbital periods. Typical values for SSs are in theorder of years, whereas for CVs they are of a few hours. Both systems undergounpredictable outbursts, characterized by a brightening in the optical by 1 - 3and 7 - 15 mag for SSs and CVs, respectively. By modelling the multiwavelengthSED of selected examples from both groups of these interacting binaries, Idetermine their basic physical parameters at a given time of the outburstevolution. In this way I show that the principal difference between outburstsof these objects is their violence, whereas the ionization structure of theirejecta is basically very similar. This suggests that the mechanism of the massejection by the white dwarfs in these systems is also similar.

On the diversity and similarity of outbursts of symbiotic binaries and cataclysmic variables