Radio and X-ray study of cygnus A
ASTROPHYS SPACE SCI 311:1-3 (2007) 323-327
Abstract:
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.The empirical metallicity dependence of the mass-loss rate of O- and early B-type stars*
Astronomy & Astrophysics EDP Sciences 473:2 (2007) 603-614
The first polarimetric signatures of infrared jets in X-ray binaries
(2007)