SUMMARY OF PROPOSAL 51087

DR YUICHI KAMATA
KAMATA@SATIO.PHYS.NAGOYA-U.AC.JP

NAGOYA UNIVERSITY
AICHI-KEN JAPAN 464-01
NAGOYA-SHI
FURO-CHO, CHIKUSA-KU
Tel: 052-789-2921 Fax: 052-789-2919
Medium: 4GBDAT
Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION

STRONG EMISSION LINE OBJECT DESCOVERD BY THE GALACTIC SURVEY


ABSTRACT

Hard X-ray source was detected during the Galactic Ridge observation program of ASCA in Mar/1996. The source shows irregular shape in the X-ray image and the spectrum shows intense Si and Fe line which are equivalent to more than 3 times cosmic value assuming various plasma temperatures. To seek out the nature of this weak X-ray source, we propose 80ks in AO5 by ASCA.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
SHIGEO YAMAUCHIIWATE UNIVERSITYJAPAN
TOMOYOSHI MAEDAKYOTO UNIVERSITYJAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)HARD_RIDGE_SOURCE
3
263.8333-32.6272 40 ksN
Y
P
0.10000
1