SUMMARY OF PROPOSAL 61064
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 KINUGASA | OSAKA UNIV. | JAPAN |
MASANOBU OZAKI | ISAS | JAPAN |
MASAAKI SAKANO | KYOTO UNIV. | JAPAN |
TADAYASU DOTANI | ISAS | JAPAN |
HIROSHI TSUNEMI | OSAKA UNIV. | JAPAN |
KENICHI TORII | OSAKA UNIV. | JAPAN |
NOBUYUKI KAWAI | RIKEN | JAPAN |
TAKASHI TONORI | OSAKA UNIV. | JAPAN |
TARGETS
TARGET NAME | PRI | RA | DEC | TIME | TC | OFF | GIS | SIS CNT | OBS |
---|
1)G352.7-0.1 | 3 | 261.9000 | -35.1167 | 40 ks | N | Y | P | 0.03000 | 1 |