scholarly journals Starburst radio galaxies: general properties, evolutionary histories and triggering

Author(s):  
C. Tadhunter ◽  
J. Holt ◽  
R. González Delgado ◽  
J. Rodríguez Zaurín ◽  
M. Villar-Martín ◽  
...  
1996 ◽  
pp. 311-312
Author(s):  
U. Klein ◽  
K.-H. Mack ◽  
L. Saripalli

2014 ◽  
Vol 570 ◽  
pp. A97 ◽  
Author(s):  
Y. I. Izotov ◽  
N. G. Guseva ◽  
K. J. Fricke ◽  
E. Krügel ◽  
C. Henkel

1996 ◽  
Vol 175 ◽  
pp. 311-312
Author(s):  
U. Klein ◽  
K.-H. Mack ◽  
L. Saripalli

So far, the number of so-called giant radio galaxies (GRGs) is small. We define them as radio sources with linear sizes larger than 1 Mpc (H0 = 75 km s–1 Mpc–1). On-going low-frequency surveys may come up with many more candidates for this species. Their very existence may ultimately be connected with their environment. For instance, for a source like 3C236, which exhibits a linear and undisturbed structure over some 4 Mpc, the surrounding medium must have a low density. GRGs may thus serve to probe large volumes of the most tenuous intergalactic medium (IGM), e.g. via depolarization studies.


1986 ◽  
Vol 64 (4) ◽  
pp. 392-397 ◽  
Author(s):  
Wil van Breugel

Observations of radio galaxies that have extended optical emission-line regions provide a new way of studying the interaction of extragalactic jets with their ambient medium. Their general properties are briefly reviewed and are illustrated using recent results on 4C 29.30 and Minkowski's Object.


2016 ◽  
Vol 824 (2) ◽  
pp. 94 ◽  
Author(s):  
Santi Roca-Fàbrega ◽  
Octavio Valenzuela ◽  
Pedro Colín ◽  
Francesca Figueras ◽  
Yair Krongold ◽  
...  

2001 ◽  
Vol 1 ◽  
pp. 131-144
Author(s):  
B. Rocca-Volmerange
Keyword(s):  

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