High-sensitivity radio observations of the Coma cluster of galaxies

1990 ◽  
Vol 99 ◽  
pp. 1381 ◽  
Author(s):  
T. Venturi ◽  
G. Giovannini ◽  
L. Feretti
Keyword(s):  
High Sensitivity ◽  
Coma Cluster ◽  
Radio Observations ◽  
Cluster Of Galaxies

scholarly journals A deep wide survey of faint low surface brightness galaxies in the direction of the Coma cluster of galaxies

2006 ◽  
Vol 459 (3) ◽  
pp. 679-692 ◽  
Author(s):  
C. Adami ◽  
R. Scheidegger ◽  
M. Ulmer ◽  
F. Durret ◽  
A. Mazure ◽  
...  
Keyword(s):  
Surface Brightness ◽  
Coma Cluster ◽  
Cluster Of Galaxies ◽  
Low Surface Brightness ◽  
Low Surface Brightness Galaxies

High Sensitivity Radio Observations of NGC 4151

1992 ◽  
pp. 338-344 ◽  
Author(s):  
A. Pedlar ◽  
M. Kukula ◽  
D. Longley ◽  
D. Axon ◽  
S. Baum ◽  
...  
Keyword(s):  
High Sensitivity ◽  
Radio Observations ◽  
Ngc 4151

scholarly journals Radio Observations of Small Diameter Sources in the Direction of Old Supernova Remnants

1983 ◽  
Vol 101 ◽  
pp. 287-288
Author(s):  
E. Fürst ◽  
W. Reich ◽  
W. Hirth
Keyword(s):  
Star Formation ◽  
Supernova Remnants ◽  
Small Diameter ◽  
High Sensitivity ◽  
Interstellar Matter ◽  
Radio Observations ◽  
Physical Association

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.

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