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   PR # 41022
   With the ASCA AO2 observation, we found that the proto-satr candidate
   R1 in the Rcr B Cloud exhibited hard X-ray emission and flare
   activities. The X-ray spectrum of R1 is very unusual with an
   emission-line-pair at 6.2 keV and 6.8 keV. R1 has been known to have
   radio Jet. However its velocity may not be larger than 100 km/sec,
   hence impossible to produce the 6.2 and 6.9 keV lines by the doppler
   shift. To confrim this peculiar phenomenon and to see possible change
   of the "doppler shifted" energy, we propose to observe R1 again. Also
   we propose an observation of IRAS162923-22, which shows almost
   identical apearence to R1 in the radio band.
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