Young Stars and Planets Near the Sun: Explosive Phenomena from Falling Evaporating Bodies

Impacts of falling evaporating bodies (FEBs) with stars and planets at velocities V >~ 10 - 20 km/s will be accompanied, due to aerodynamic effects such as crushing and transversal expansion of the crushed mass, by the FEB's ``explosion'' and the generation of a strong ``blast'' wave, resulting in FEB-generated explosive/flare phenomena. Multiwavelength monitoring of nearby young stars (and exoplanets) with dense protoplanetary disks rich in FEB's is hence of interest for identifying such FEB-related mechanisms possibly underlying their variability.