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Fig. 5


Influence of stellar spots included in our model on the radial velocity curve of the primary (top) and secondary (bottom) components of ASAS-09 (left) and ASAS-21 (right) systems. ASAS-09 models were constructed with one spot and ASAS-21 with two spots (one on each component). Solid lines depict the base solution which in the case of ASAS-21 is represented by the configuration, with two eclipsed spots. Points with errorbars are the residua of the orbital fit. Their coding is the same as in Fig. 2.

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