SUMMARY OF PROPOSAL 51097

MR. YOSHITOMO MAEDA
MAEDA@CR.SCPHYS.KYOTO-U.AC.JP

KYOTO UNIVERSITY
KYOTO JAPAN 606-01
KYOTO
KITASHIRAKAWA-OIWAKE-CHO SAKYO-KU
Tel: 075-753-3843 Fax: 075-701-5377
Medium: 2.5GB8MM
Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION

SEARCH FOR THE GALACRIC DIFFUSE EMISSION


ABSTRACT

We observe three positions in the Galactic Bulge: (0 deg, -5 deg) (0 deg, -7 deg) (0 deg, -11 deg). The Bulge plasma will be due to the expansion of the plasma heated up near the Galactic Center. We have an evidence of changing of the temperature during AO3 and AO4 phase. During the AO5 phase, we look for the tempature, density, pressure and abundance of the Bulge plasma. We will study the mechanizem of the import of interstellar high temparature gases.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
KATSUJI KOYAMAKYOTO UNIVERSITYJAPAN
YASUO TANAKAMPEGERMANY
KEN EBISAWAGSFCUSA
SHIGEO YAMAUCHIIWATE UNIVERSITYJAPAN
MASAAKI SAKANOKYOTO UNIVERSITYJAPAN
MAMIKO NISHIUCHIKYOTO UNIVERSITYJAPAN
FRANK MARSHALLGSFCUSA

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)(0 DEG, -5 DEG)
2
271.4075-31.4487 40 ksN
N
P
1.00000
1
2)(0 DEG, -7 DEG)
2
273.4817-32.3981 40 ksN
N
P
1.00000
1

TARGET 1

WE HOPE THAT OUR OBSERVATION WILL BE PERFORMED DURING THE SPRING 1997 OBSEVATION WINDOW..

TARGET 2

WE HOPE THAT OUR OBSERVATION WILL BE PERFORMED DURING THE SPRING 1997 OBSEVATION WINDOW..