SUMMARY OF PROPOSAL 61074

MASTER TATSUHIKO ASANUMA
ASANUMA@ESS.SCI.OSAKA-U.AC.JP

OSAKA UNIVERSITY
OSAKA JAPAN 560
TOYONAKA
MACHIKANEYAMA-CHO 1-1
Tel: 06-850-5476 Fax: 06-850-5539
Medium: 2.5GB8MM
Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION

OBSERVATION OF COMPOSITE TYPE SNRS G116.5+11 & G117.4+5


ABSTRACT

We propose the observation of composite type SNR G116.5+1.1 and G117.4+5 . The morphology of these SNR's are shell type in radio and are center filled type in X-ray. This class of SNR's has been revealed to emitting thermal spectrum in X-ray. ASCA's observation shows these spacally resolved spectra are not uniform. We found the gradience of metal abundances in spece. We want to determin the origin of this class of SNR, evaporation or remaining ejecta, through getting the gradience of metal abundance of each heavy element from spacally resolved spectorum.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
EMI MIYATAOSAKA UNIV.JAPAN
KENICHI TORIIOSAKA UNIV.JAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)G117.4+5
3
359.5421 67.5657 30 ksN
Y
P
0.40000
1