High-sensitivity radio observations of the Coma cluster of galaxies

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

1968 ◽  
Vol 152 ◽  
pp. L155 ◽  
Author(s):  
E. P. Bozyan




1984 ◽  
Vol 305 (4) ◽  
pp. 175-185 ◽  
Author(s):  
F. W. Baier


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






1992 ◽  
pp. 338-344 ◽  
Author(s):  
A. Pedlar ◽  
M. Kukula ◽  
D. Longley ◽  
D. Axon ◽  
S. Baum ◽  
...  


1983 ◽  
Vol 101 ◽  
pp. 287-288
Author(s):  
E. Fürst ◽  
W. Reich ◽  
W. Hirth

Radio observations with high sensitivity have shown that lots of more or less compact structures can be found in the field of extended and old supernova remnants (SNRs). These small diameter sources have been subject to many recent observations. The aim of these studies is to infer a possible physical association of these sources with the SNR shell. The interest in this link is based on various aspects, instabilities of shocked interstellar matter, star formation, etc.



1990 ◽  
Vol 105 (8-9) ◽  
pp. 845-856
Author(s):  
Kwang-Tae Kim


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