SUMMARY OF PROPOSAL 41022
DR. KATSUJI KOYAMA
KYOTO UNIV.
KYOTO JAPAN 606-01
KYOTO
KITASHIRAKAWA

  E-mail: TSUBOI@CR.SCPHYS.KYOTO-U.AC.JP	Tel: (81)-75-753-3843	Fax: (81)-75-701-5377
  Medium: 2.5GB8MM

Subject: STARS                                                       
  Title: OBSERVATIONS OF NEW JET-OBJECTS                                                 


Abstract:
 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.

 Co-Is:
   1  Y. TSUBOI           	KYOTO UNIV.                   JAPAN     
      (No Co-I contact data)
   2  S. UENO             	KYOTO UNIV.                   JAPAN     
   3  N. KOBAYASHI        	NAO                           JAPAN     
   4  M. HAYASHI          	NAO                           JAPAN     
   5  S. YAMAUCHI         	IWATE UNIV                    JAPAN     


Target Name           PRI RA        Dec        Time TC  Off GIS SIS_Cts  Obs
-------------------   --- --------  --------   ---- --  --- --- -------  ---
R CR A                 1  285.4817  -36.9527    80   N   Y   P  0.10000   1 
          
RHO OPH EAST           1  248.0942  -24.4756    20   N   Y   P  0.10000   1