SUMMARY OF PROPOSAL 61126

PROF. 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 Fax: 0427-59-4253
Medium: 2.5GB8MM
Subject: AGN

A 200 KS ASCA OBSERVATION OF THE BROAD IRON LINE IN THE RADIO GALAXY 3C120


ABSTRACT

We propose to observe the radio galaxy 3C120 to see any similarities and/or differences in the line profile from those of Seyfert 1 galaxies and to see whether or not the broad, skewed, profile of the iron line is really emission from matter within a few Schwarzschild radii of a black hole. According the previous ASCA observation of this source, we will be able to have a line profile with the same quality as that of MCG-6-30-15 by a 200 ks observation. From a constraint on the inclination angle of jets of this source given by the superluminal motion, we will be able to discuss the origin of the line profile in terms of the diks-line model. At the same time, it might be possible to see changes of the innermost accretion disk associated with the jet-activity.

CO-INVESTIGATORS
CO-I NAME INSTITUTE COUNTRY
FUMIYOSHI MAKINOISASJAPAN
MANABU ISHIDAISASJAPAN
RYUICHI FUJIMOTOISASJAPAN
MASARU MATSUOKARIKENJAPAN
CHIKO OTANIRIKENJAPAN
HIDEYO KUNIEDANAGOYA UNIV.JAPAN
HISAMITSU AWAKIKYOTO UNIV.JAPAN
KOYOSHI HAYASHIDAOSAKA UNIV.JAPAN
AKIKO YAMASHITAISASJAPAN
YUICHI TERASHIMANAGOYA UNIV.JAPAN

TARGETS

TARGET NAMEPRIRADECTIMETCOFFGISSIS CNTOBS
1)3C120
2
68.2963 5.3543 100 ksN
Y
P
1.90000
1