SUMMARY OF PROPOSAL 41210
 SHIRO UENO
KYOTO UNIVERSITY
KYOTO JAPAN 606-01
KYOTO
SAKYO-KU

  E-mail: UENO@CR.SCPHYS.KYOTO-U.AC.JP	Tel: +81-75-753-3869	Fax: +81-75-701-5377
  Medium: 2.5GB8MM

Subject: AGN                                                         
  Title: DISTRIBUTION OF MATTER AROUND QUASAR'S NUCLEI (RADIO-LOUD QUASAR)               


Abstract:
 The radio-loud quasars, PKS0312-77 and 3C249.1 are classified as "core dominant" and
 as "lobe dominant" respectively, depending on the ratio of radio fluxes from the
 "core" of the AGN and the "lobes". The core dominance indicates an alignment of the
 jet of AGN and our line of sight. Thus comparison of spectra and time variability
 between these objects provides a good chance to investigate the distribution of
 matter around quasars and X-ray beaming. A correlation between photon-index and core
 dominance is suggested with the Einstein in the limited energy band. The
 establishment requires ASCA observations to estimate the contribution from the
 absorption and soft thermal component etc. Moreover ASCA can resolve difficlulties
 in the study of beaming by using the Fe-K line.

 Co-Is:
   1  HISAMITSU AWAKI     	KYOTO UNIVERSITY              JAPAN     
      (No Co-I contact data)
   2  KATSUJI KOYAMA      	KYOTO UNIVERSITY              JAPAN     


Target Name           PRI RA        Dec        Time TC  Off GIS SIS_Cts  Obs
-------------------   --- --------  --------   ---- --  --- --- -------  ---
3C249.1                3  166.0579   76.9828    40   N   Y   P  0.29300   1