SUMMARY OF PROPOSAL 61080
KYOTO UNIVERSITY
KYOTO JAPAN 606-01
KYOTO
KITASHIRAKAWA-OIWAKE-CHO SAKYO-KU
Tel: +81-75-753-3867 Fax: +81-75-701-5377
Medium: 2.5GB8MM
Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION
A TREASURY OF X-RAY SOURCES: (L,B)
ABSTRACT
We have observed the Galactic Center region with ASCA, and got many fruitful results. The region around (l,b)=(359,-1) is the special region where many high-energy phenomena are known, but not observed with ASCA. In this region, there are peculiar radio non-thermal structure "the Mouse", two X-ray bursters SLX 1744-299/300, and shell-type SNR G359.0-0.9. Our goal is solving each physics of them on the viewpoint of high energy phenomena, and then finding the phenomena or laws which can be applied to the whole Galactic Center region. Especially, our first objective is detecting the hard X-ray emission corresponding to the Mouse, solving the emission mechanism and its origin.
CO-INVESTIGATORS
| CO-I NAME | INSTITUTE | COUNTRY |
|---|
| KATSUJI KOYAMA | KYOTO UNIVERSITY | JAPAN |
| YOSHITOMO MAEDA | KYOTO UNIVERSITY | JAPAN |
| JUN YOKOGAWA | KYOTO UNIVERSITY | JAPAN |
| MAMIKO NISHIUCHI | KYOTO UNIVERSITY | JAPAN |
| HIROSHI MURAKAMI | KYOTO UNIVERSITY | JAPAN |
TARGETS
| TARGET NAME | PRI | RA | DEC | TIME | TC | OFF | GIS | SIS CNT | OBS |
|---|
| 1)THE MOUSE | 2 | 266.8133 | -29.9667 | 80 ks | N | N | P | 2.00000 | 1 |
TARGET 1
WE HOPE THAT THE OBSERVATION WILL BE MADE IN FALL, BECAUSE WE HOPE THAT THE CENTER OF FIELD OF VIEW IS NEAR G359.0-0.9 (RA,DEC)=(266.81,-30.11) AND APART FROM A1742-294 (266.52,-29.50) IN J2000.