SUMMARY OF PROPOSAL 41082
MR. ICHIZO HAYASHI
KYOTO UNIVERSITY
KYOTO JAPAN 606-01
KYOTO
KITASHIRAKAWAOIWAKE-CHO SAKYO-KU

  E-mail: HAYASHI@CR.SCPHYS.KYOTO-U.AC.JP	Tel: +81-75-753-3851	Fax: +81-75-701-5377
  Medium: 2.5GB8MM

Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION            
  Title: SUPERNOVA REMNANTS IN THE WIND-BLOWN BUBBLES                                    


Abstract:
 The evolution and characteristics of supernova remnants are considered to be
 affected by the circumstellar environment of progenitor stars. In particular,
 wind-blown bubbles created by the steller wind of massive stars will have
 significant effect on supernova remnants in that bubbles. Although these remnants
 are difficult to be observed because of their low X-ray brightness and the
 contamination by surrounding HII regions, the Einstein satellite detected several
 supernova remnants in the giant HII regions in the Magellanic Clouds. We propose the
 first hard X-ray spectroscopy of supernova remnants clearly associated with the
 wind-blown super bubbles in the Small Magellanic Cloud.

 Co-Is:
   1  KATSUJI KOYAMA      	KYOTO UNIVERSITY              JAPAN     
      (No Co-I contact data)
   2  IKUKO ASAOKA        	MAX PLANCK INSTITUTE          GERMANY   


Target Name           PRI RA        Dec        Time TC  Off GIS SIS_Cts  Obs
-------------------   --- --------  --------   ---- --  --- --- -------  ---
N19                    3   11.8167  -73.1417    40   N   Y   P  0.13000   1 

REMARKS:           LET GIS COVER 6 SNRS AND SIS COVER 5 SNRS AROUND N19.

REMARKS:           LET SIS COVER 2 SNRS 0057-724 AND 0056-725.