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The phenomenon of microlensing has successfully been used to detectextrasolar planets. By observing characteristic, rare deviations in thegravitational microlensing light curve one can discover that a lens is astar--planet system. In this paper we consider an opposite case where the lensis a single star and the source has a transiting planetary companion. We havestudied the light curve of a source star with transiting companion magnifiedduring microlensing event. Our model shows that in dense stellar fields, inwhich blending is significant, the light drop generated by transits is greaternear the maximum of microlensing, which makes it easier to detect. We derivethe probability for the detection of a planetary transit in a microlensedsource to be of 2*10^(-6) for an individual microlensing event.

Transiting Planets Orbiting Source Stars in Microlensing Events