SUMMARY OF PROPOSAL 51035

DR. TAKESHI GO TSURU
TSURU@CR.SCPHYS.KYOTO-U.AC.JP

KYOTO
KYOTO JAPAN 606-01
KYOTO
KITASHIRAKAWA
Tel: (81)-75-753-3843 Fax: (81)-75-701-5377
Medium: 2.5GB8MM
Subject: STARS

X-RAY SPECTRA OF RED GIANT AND RED SUPER GIANT STARS


ABSTRACT

ASCA has observed only one red giant star altough ROSAT has been detecting some red, red bright and red super giant stars. However, Due to the poor energy resolution of ROSAT observatory, temperature, abundance and absorption column of X-rays from these evolved late-type stars are still unknown. Hence, no clear observational ansower to the emission and the heating mechanism has been obtained. This is the first attempt to obatin precise X-ray spectra of these stars and give a clear observational ansower to the questions.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
YOHKO TSUBOIKYOTOJAPAN
KATSUJI KOYAMAKYOTOJAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)BETA CAM
2
75.8546 60.4422 40 ksN
Y
P
0.02000
1
2)BETA GEM (POLLUX)
2
116.3287 28.0261 40 ksN
Y
P
0.01400
1