SUMMARY OF PROPOSAL 81411

MR MASAAKI SAKANO
SAKANO@CR.SCPHYS.KYOTO-U.AC.JP

KYOTO UNIVERSITY
KITASHIRAKAWA-OIWAKE-CHO SAKYO-KU
KYOTO
KYOTO JAPAN 606-8502
Tel: +81-75-753-3867 Fax: +81-75-753-3799
Medium: CD ROM
Subject: X-RAY BINARIES

EXTREMELY HARD X-RAY SOURCES IN THE GALACTIC CENTER REGION


ABSTRACT

In the Galactic Center survey, ASCA resolved many point sources in the region through the heavy interstellar absorption for the first time. Some of them were found to show unusually hard spectra. They are probably one of unusual objects, such as X-ray pulsar or black hole. In particular, one of the targets, AX J1739.1-3021, showed an extremely strong flare with more than 2-order magnitude variability in only 1000sec. We here propose the long observations of three of those unusually hard objects which have been not identified, yet. Our first objective is to detect time variability and then to reveal their natures. In addition to the interest to their natures themselves, they would give some important implication on the star formation history in the Galactic Center region.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
KATSUJI KOYAMAKYOTO UNIVERSITYJAPAN
HIROSHI MURAKAMIKYOTO UNIVERSITYJAPAN
SHIGEO YAMAUCHIIWATE UNIVERSITYJAPAN
TADAYASU DOTANIISASJAPAN
FUMIAKI NAGASEISASJAPAN
KEN'ICHI TORIINASDAJAPAN
YOSHITOMO MAEDAPEN-STATE UNIVERSITYUSA
KENZO KINUGASAGUNMA ASTRON. OBS.JAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)AXJ1739.1-3035
B
264.7833-30.3500
200 ks
N
Y
P
0.50000
1