SUMMARY OF PROPOSAL 41250
DR. KOUJUN YAMASHITA
NAGOYA UNIVERSITY
AICHI-KEN JAPAN 464-01
NAGOYA
FURO-CHO, CHIKUSA-KU

  E-mail: YAMASITA@SATIO.PHYS.NAGOYA-U.AC.JP	Tel: 81-52-789-3540	Fax: 81-52-789-2919
  Medium: 4GBDAT

Subject: CLUSTERS OF GALAXIES AND SUPERCLUSTERS                      
  Title: TEMPERATURE AND ABUNDANCE DISTRIBUTION OF RICH CLUSTERS SELECTED FROM ESO KEY PROGRAMME OBSERVATIONS


Abstract:
 It is important to investigate the formation and evolution of clusters by means of
 optical and X-ray observations. There are no good correlations between optical and
 X-ray parameters. The detailed optical observations ob Abell clusters $(z<0.1)$ in
 southern sky are carried out by ESO key programme. We have selected two rich
 clusters out of 107 A3158(z=0.0592) and A3128(z=0.0600). We make clear the
 correlation among the distribution of galaxies. ICM and dark matter in these
 clusters by combining ASCA data and ESO optical data. This gives a clue to
 investigate the \beta -problem, origin of ISM and cluster merging.

 Co-Is:
   1  YUZURU TAWARA       	NAGOYA UNIV.                  JAPAN     
      (No Co-I contact data)
   2  AKIHIRO FURUZAWA    	NAGOYA UNIV.                  JAPAN     
   3  FUMIE AKIMOTO       	NAGOYA UNIV.                  JAPAN     
   4  MANABU WATANABE     	NAGOYA UNIV.                  JAPAN     
   5  AKIKO KUMADA        	NAGOYA UNIV.                  JAPAN     
   6  SHIGERU MIYOSHI     	KYOTO SANGYO UNIV.            JAPAN     
   7  A. MAZURE           	CNRS, LAS                     FRANCE    


Target Name           PRI RA        Dec        Time TC  Off GIS SIS_Cts  Obs
-------------------   --- --------  --------   ---- --  --- --- -------  ---
A3158                  3   55.7500  -53.6333    40   N   N   P  0.80000   1