*************************************************************************
   61019
   In AO2, the protostar R1 in the R CrA star forming region shows the
   powerful X-ray flare. The flare spectrum is unusual, showing a
   broadened or double emissionline structure between 6.2 and 6.8keV. The
   reasonable explanation of this phenomina is the doppler shift of iron
   line by the jet drived by flare, but, if it does, the speed of the jet
   is comparable of the 10 % of the light speed. It is unbeliabable
   result. But, resent observation and scimulation reveals the existance
   of high speed jet around star forming region To study further, we need
   to know the precise flare parameters. So, we observe the RCrA star
   forming region again with ASCA.
 *************************************************************************