Coordinated HST-EUVE Observations of YZ CMi

The observations were taken as part of a coordinated observing campaign which was designed to study flares on the dMe star YZ CMi. The campaign also included rapid spectral time sequences in the optical (using the 3.9 m Anglo-Australian Telescope) and UV (using the GHRS aboard the Hubble Space Telescope and the IUE satellite) and radio observations taken with the Australia Telescope and VLA. The goal was to investigate the physical characteristics of the flares in different temperature regimes with a time resolution which is high enough to investigate the dynamics of the events.