SUMMARY OF PROPOSAL 61066

MR HIDEHIRO KANEDA
KANEDA@MIRANDA.PHYS.S.U-TOKYO.AC.JP

UNIVERSITY OF TOKYO
TOKYO JAPAN 113
BUNKYO-KU
7-3-1 HONGO
Tel: 03-3812-2111 EX4173 Fax: 03-3812-6938
Medium: 2.5GB8MM
Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION

HIGH-LATITUDE EMISSION OF THE GALACTIC RIDGE X-RAYS


ABSTRACT

We propose to observe the off-plane regions of the Scutum Arm (l = 28) at the latitudes of b = 3--4 deg. From the past observations with ASCA, we detected another diffuse faint non-thermal-like component in addition to the well-known GRXE thermal component of temperature kT = 3--10 keV. This powerlaw-like component extends toward higher latitudes than the thermal component. GINGA also detected a similar "hard tail" component in the Galactic ridge X-ray spectra. Therefore, it is highly possible that the power-like component is identical with the "hard tail" and thus truly of non-thermal origin. In order to further discuss the origin of the power-like component, we need off-plane observations at higher latitudes.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
KAZUO MAKISHIMAUNIVERSITY OF TOKYOJAPAN
KEIICHI MATSUZAKIUNIVERSITY OF TOKYOJAPAN
SHIGEO YAMAUCHIIWATE UNIVERSITYJAPAN
NORIKO YAMASAKITOKYO METRO. UNIV.JAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)GALACTIC OFF-PLANE#1
2
278.1054 -2.8814 20 ksN
Y
P
0.04000
1
2)GALACTIC OFF-PLANE#2
2
278.3808 -2.3492 20 ksN
Y
P
0.04000
1
3)GALACTIC OFF-PLANE#3
2
277.5721 -2.6055 20 ksN
Y
P
0.04000
1
4)GALACTIC OFF-PLANE#4
2
277.8475 -2.0736 20 ksN
Y
P
0.04000
1