Radio and X-ray study of Cygnus A
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 s...
Principais autores: | Steenbrugge, K, Blundell, K |
---|---|
Formato: | Journal article |
Idioma: | English |
Publicado em: |
2007
|
Registros relacionados
-
Radio and X-ray study of Cygnus a
por: Steenbrugge, K, et al.
Publicado em: (2007) -
Radio and X-ray study of cygnus A
por: Steenbrugge, K, et al.
Publicado em: (2007) -
Detection of a relic X-ray jet in Cygnus A
por: Steenbrugge, K, et al.
Publicado em: (2007) -
Multiwavelength study of Cygnus A I. Precession and slow jet speeds from
radio observations
por: Steenbrugge, K, et al.
Publicado em: (2008) -
Multiwavelength study of Cygnus A II. X-ray inverse-Compton emission
from a relic counterjet and implications for jet duty-cycles
por: Steenbrugge, K, et al.
Publicado em: (2008)