SUMMARY OF PROPOSAL 61103

MISS KUMI YOSHITA
KYOSHITA@ESS.SCI.OSAKA-U.AC.JP

FUCULTY OF SCIENCE, OSAKA UNIVERSITY
OSAKA JAPAN 560
TOYONAKA
1-1, MACHIKANEYAMA-CHO
Tel: 06-850-5476 Fax: 06-850-5539
Medium: 2.5GB8MM
Subject: NORMAL GALAXIES

OBSERVATION OF THE SMC


ABSTRACT

So far ASCA observed E0102-72 which is half degree away from the center of the Small Magellanic Cloud(SMC). The clear enhancement was detected between E0102-72 and the center of the SMC, and it suggests the tail part of the hot component in the center. It may correspond to the Galacitc Ridge X-ray emission observed in the Galaxy. We propose to observe the hot gas structure from the center to the north part of the SMC.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
HIROSHI TSUNEMIOSAKA UNIVERSITYJAPAN
KEN'ICHI TORIIOSAKA UNIVERSITYJAPAN
EMI MIYATAOSAKA UNIVERSITYJAPAN
KENZO KINUGASAOSAKA UNIVERSITYJAPAN
TATSUHIKO ASANUMAOSAKA UNIVERSITYJAPAN
TAKASHI TONERIOSAKA UNIVERSITYJAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)SMC CENTER
3
13.4000-72.7000 40 ksN
N
P
0.20000
1