scholarly journals Extended and Compact X‐Ray Emission from the Powerful Radio Galaxy 3C 220.1

1998 ◽  
Vol 504 (2) ◽  
pp. 743-748 ◽  
Author(s):  
M. J. Hardcastle ◽  
C. R. Lawrence ◽  
D. M. Worrall
1997 ◽  
Vol 286 (3) ◽  
pp. 765-770 ◽  
Author(s):  
S. W. Allen ◽  
A. C. Fabian ◽  
E. Idesawa ◽  
H. Inoue ◽  
T. Kii ◽  
...  

1994 ◽  
Vol 47 (5) ◽  
pp. 615 ◽  
Author(s):  
DE Harris

Using a sea interferometer, Bolton and Stanley isolated Cygnus A as a discrete source in 1948. It is a prime example� of a powerful radio galaxy and, in the last decade, has also been studied extensively in X-rays. In this paper I summarise the results from a ROSAT X-ray image.


1999 ◽  
Vol 306 (2) ◽  
pp. 467-472 ◽  
Author(s):  
K. Iwasawa ◽  
S. W. Allen ◽  
A. C. Fabian ◽  
A. C. Edge ◽  
S. Ettori

2020 ◽  
Vol 20 (8) ◽  
pp. 122
Author(s):  
Lin-Hui Wu ◽  
Qing-Wen Wu ◽  
Jian-Chao Feng ◽  
Ru-Sen Lu ◽  
Xu-Liang Fan

2011 ◽  
Vol 415 (4) ◽  
pp. 3520-3530 ◽  
Author(s):  
J. Hlavacek-Larrondo ◽  
A. C. Fabian ◽  
J. S. Sanders ◽  
G. B. Taylor

2002 ◽  
Vol 19 (1) ◽  
pp. 69-72 ◽  
Author(s):  
Nectaria A. B. Gizani ◽  
M. A. Garrett ◽  
J. P. Leahy

AbstractWe present the kpc-scale behaviour of the powerful extragalactic radio source Hercules A and the behaviour of the intracluster gas in which the radio source is situated. We have found that Hercules A exhibits a strong Laing-Garrington effect. The X-ray observations have revealed an extended X-ray emission elongated along the radio galaxy axis. The estimated temperature of the cluster is kT=2.45 keV and the central electron density is n○≃7.8×10−3 cm−3 which reveals a hot, dense environment in which Hercules A is situated. From the combined study of the radio and X-ray data we have estimated a central value of 3 ≲ B○(μG)≲9.We also present the most recent results from the analysis of the radio data on the pc-scale structure of the radio galaxy, observed at 18 cm by the EVN–MERLIN array. A faint but compact radio source, coincident with the optical centre of Hercules A, was detected by the EVN at 18 mas resolution. The total flux density of the EVN core is 14.6 mJy. Its angular size is 18×7 mas with a position angle of ≃139°. There is also evidence for extended emission in the NW–SE direction, most probably from the eastern pc-scale jet. If this is true then there is a misalignment between the direction of the pc-eastern and the aligned kpc-scale jets of ≃35°.


2011 ◽  
Vol 734 (2) ◽  
pp. L28 ◽  
Author(s):  
J. H. Croston ◽  
M. J. Hardcastle ◽  
B. Mingo ◽  
D. A. Evans ◽  
D. Dicken ◽  
...  

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