SUMMARY OF PROPOSAL 61064

DR SHIGEO YAMAUCHI
YAMAUCHI@HIRYU.HSS.IWATE-U.AC.JP

IWATE UNIVERSITY
IWATE JAPAN 020
MORIOKA
3-18-34, UEDA
Tel: 81-196-21-6817 Fax: 81-196-21-6715
Medium: 4GBDAT
Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION

X-RAY OBSERVATION OF G352.7-0.1


ABSTRACT

We discovered an X-ray emission from supernova remnant, G352.7-0.1, during the galactic plane survey program performed in the AO-4 period for the first time. The diameter was about 6-8 arcmin. The X-ray spectrum shows that emission lines from Si, S, and Ar is very strong and the GIS spectrum and image imply that there is a point-like source at the center. However, since the exposure time during the survey program was short, we could not obtain statistically good data. Thus, we propose a follow-up observation of this supernova remnant.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
KENZO KINUGASAOSAKA UNIV.JAPAN
MASANOBU OZAKIISASJAPAN
MASAAKI SAKANOKYOTO UNIV.JAPAN
TADAYASU DOTANIISASJAPAN
HIROSHI TSUNEMIOSAKA UNIV.JAPAN
KENICHI TORIIOSAKA UNIV.JAPAN
NOBUYUKI KAWAIRIKENJAPAN
TAKASHI TONORIOSAKA UNIV.JAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)G352.7-0.1
3
261.9000-35.1167 40 ksN
Y
P
0.03000
1