SUMMARY OF PROPOSAL 41078
PROFESSOR HIROSHI TSUNEMI
FACULTY OF SCIENCE, OSAKA UNIVERSITY
OSAKA JAPAN 560
TOYONAKA
1-1, MACHIKANEYAMA

  E-mail: TSUNEMI@ESS.SCI.OSAKA-U.AC.JP	Tel: 06-850-5477	Fax: 06-850-5539
  Medium: 2.5GB8MM

Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION            
  Title: OBSERVATION OF G69.7+1.0 AND G7.7-3.7 DETECTED BY ROSAT                         


Abstract:
 We propose to observe two SNRs that are newly discovered with Rosat. They are
 G69.7+1.0 and G7.7-3.7. G69.7+1.0 shows an extended structure parallel to the
 galactic plane suggesting the hot bubble prevailing in the galaxy. G7.7-3.7 shows a
 shell structure with asymmetric X-ray brightness. Since they are dim in radio, they
 have not been observed before the Rosat era. They may form a new type of SNR groups.

 Co-Is:
   1  KENZO KINUGASA      	OSAKA UNIV.                   JAPAN     
      KINUGASA@ESS.SCI.OSAKA-U.AC.JP	06-850-5476
   2  EMI MIYATA          	OSAKA UNIV.                   JAPAN     
   3  TATSUHIKO ASANUMA   	OSAKA UNIV.                   JAPAN     
   4  KEN'ICHI TORII      	OSAKA UNIV.                   JAPAN     


Target Name           PRI RA        Dec        Time TC  Off GIS SIS_Cts  Obs
-------------------   --- --------  --------   ---- --  --- --- -------  ---
G69.7+1.0              3  300.6750   32.7167    40   N   N   P  0.57000   3 

REMARKS:  1ST POINTING : (20H02M42S,32D43M00S) : 0.57CPS/SIS : 15KSEC\\ 2ND POINTING
          : (20H01M30S,32D31M00S) : 0.32CPS/SIS : 10KSEC\\ 3RD POINTING :
          (20H00M45S,32D54M00S) : 0.52CPS/SIS : 15KSEC\\