SUMMARY OF PROPOSAL 51080

DR. HAJIME INOUE
INOUE@astro.isas.jaxa.jp

INSTITUTE OF SPACE AND ASTRONAUTICAL SCIENCE
KANAGAWA JAPAN 229
SAGAMIHARA
3-1-1 YOSHINODAI
Tel: 0427-51-3911(2615) Fax: 0427-59-4253
Medium: 2.5GB8MM
Subject: SUPERNOVA REMNANTS AND GALACTIC DIFFUSE EMISSION

OBSERVATIONS OF SN1993J


ABSTRACT

SN 1993J is one of five recent supernova explosions (SNe) detected in X-rays. It is observationally unprecedented, in that it is the only SNe detected in the radio and in X-rays within a week of the explosion, and whose X-ray light curve and spectral evolution have been carefully measured for over one year. We detected X-ray intensity variations in last one year, which is faster than we expect from a shock heating models. Thus, continuous monitoring is urged. We also expect to detect emission from a pulsar, if it is as bright as Crab pulsar.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
WALTER H.G. LEWINMITUSA
YASUO TANAKAMPEJAPAN
KAZUO MAKISHIMATOKYO. UNIV.JAPAN
SHIN'ICHIRO UNOISASJAPAN
KAZUHISA MITSUDAISASJAPAN
TADAYUKI TAKAHASHIISASJAPAN
DEREK FOXMITUSA
MASAYUKI ITOHKOBE. UNIV.JAPAN
YOSHIKI KOHMURARIKENJAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)SN1993J
1
148.8542 69.0202 100 ksN
Y
P
0.02000
2

TARGET 1

50 KS DURING MARCH 12 - MAY 31 1997 \ 50 KS DURING SEPT.14 - DEC 3 1997