SUMMARY OF PROPOSAL 61004

MS. TAE FURUSHO
FURUSHO@PHYS.METRO-U.AC.JP

TOKYO METROPOLITAN UNIVERSITY
TOKYO JAPAN 192-03
HACHIOJI
1-1, MINAMI-OSAWA
Tel: +81-426-77-2485 Fax: +81-426-77-2483
Medium: 4GBDAT
Subject: STARS

STUDY OF X-RAY EMISSION FROM CLASS 0 PROTOSTAR


ABSTRACT

X-ray observation of class 0 protostar, L1157 is proposed. ASCA detected X-ray emission from Class I protostars for the first time. The origin of the X-ray emission from protostars is very unclear, however, the X-ray emission gave us very impotant information about star formation, for example about rotaion, and magnetic field. The proposed taeget L1157 at a distance of 440pc has well-collimated bipolar outflows which cause strong shock-heating of the ambient gas.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
NORIKO YAMASAKITOKYO METRO. UNIV.JAPAN
YUTARO SEKIMOTOUNIV. OF TOKYOJAPAN
TOMOFUMI UMEMOTONAOJAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)L1157
2
309.7742 68.0379 60 ksN
Y
P
0.05000
1