Radio and X-ray study of Cygnus A

Details Radio and X-ray study of Cygnus A Radio and X-ray study of Cygnus A

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.310..321s&link_type=abstract

Astrophysics and Space Science, Volume 310, Issue 3-4, pp. 321-325

Astronomy and Astrophysics

Astrophysics

2

Galaxies: Active, Galaxies: Jets, Galaxies:&Nbsp, X-Ray, Galaxies: Radio

Scientific paper

We present a comparative analysis of 5 GHz VLA and 200 ks Chandra ACIS-I image. In the 5 GHz image the familiar jet and much weaker counterjet are seen, which bend as the jet propagates towards the hotspots. Furthermore, where the lobe detected in 5 GHz emission starts to interact with the jet, we see that the jet “threads”. In the 0.2 10 keV X-ray image we do not detect the jet, but do detect a relic of the counterjet.

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