Detection of a Temperature Structure in the Coma Cluster of Galaxies with [ITAL]ASCA[/ITAL]

1996 ◽  
Vol 473 (2) ◽  
pp. L71-L74 ◽  
Author(s):  
H. Honda ◽  
M. Hirayama ◽  
M. Watanabe ◽  
H. Kunieda ◽  
Y. Tawara ◽  
...  
1998 ◽  
pp. 308-309 ◽  
Author(s):  
H. Honda ◽  
M. Hirayama ◽  
H. Ezawa ◽  
K. Kikuchi ◽  
T. Ohashi ◽  
...  

1998 ◽  
Vol 188 ◽  
pp. 308-309
Author(s):  
H. Honda ◽  
M. Hirayama ◽  
H. Ezawa ◽  
K. Kikuchi ◽  
T. Ohashi ◽  
...  

The Coma cluster has been recognized as an archetype of rich and relaxed clusters, until recent ROSAT observations reveal that the intracluster medium (ICM) has a complex distribution (Briel et al. 1992; White et al. 1993). The X-ray surface brightness distribution shows a secondary peak around the galaxy NGC 4839, at 40' SW from the cluster center.


2006 ◽  
Vol 459 (3) ◽  
pp. 679-692 ◽  
Author(s):  
C. Adami ◽  
R. Scheidegger ◽  
M. Ulmer ◽  
F. Durret ◽  
A. Mazure ◽  
...  

1990 ◽  
Vol 99 ◽  
pp. 1381 ◽  
Author(s):  
T. Venturi ◽  
G. Giovannini ◽  
L. Feretti

1990 ◽  
Vol 355 ◽  
pp. 29 ◽  
Author(s):  
K.-T. Kim ◽  
P. P. Kronberg ◽  
P. E. Dewdney ◽  
T. L. Landecker

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