... Notes: Has been called G332.4+0.2. Radio: Distorted shell, with thermal jet and plume adjacent. Optical: Detected. X-ray: Shell, brightest to NW. ...
... Optical: Faint filaments. X-ray: Centrally brightened, with faint jet. Point sources: Central pulsar. Distance: H I absorption indicates 2 kpc. ...
... X-ray: Partial shell, central nebula and pulsar and `jet'. Point sources: Radio and X-ray pulsar, with wind nebula. ... ADS . Yatsu et al. 2005, ApJ, 631, 312. Chandra observations of pulsar and jet. ADS . DeLaney et al. 2006, ApJ, 640, 929. ...
... Optical: Fast knots and quasi-stationary flocculli, with many filaments at large radii, and NE `jet'. ... Laming et al. 2006, ApJ, 644, 260. Chandra observations, particularly of NE `jet'. ADS . Fesen et al. 2006, ApJ, 645, 283. ...
... X-ray: Partial shell, central nebula and pulsar and `jet'. Point sources: Radio and X-ray pulsar, with wind nebula. ... ADS . Yatsu et al. 2005, ApJ, 631, 312. Chandra observations of pulsar and jet. ADS . DeLaney et al. 2006, ApJ, 640, 929. ...
... Large scale simulations of the jet-IGM interaction . M.Krause . ... A 3D Hydrodynamic Simulation for the Cygnus A Jet as a Prototype for High Redshift ... Reliability of astrophysical jet simulations in 2D . M.Krause & M.Camenzind . ...
... Optical: Fast knots and quasi-stationary flocculli, with many filaments at large radii, and NE `jet'. ... ADS . Fesen & Gunderson 1996, ApJ, 470, 967. Optical observations of NE `jet'. ADS . Schwarz et al. 1997, A&AS, 123, 43. ...
... Optical: Fast knots and quasi-stationary flocculli, with many filaments at large radii, and NE `jet'. ... ADS . Fesen & Gunderson 1996, ApJ, 470, 967. Optical observations of NE `jet'. ADS . Schwarz et al. 1997, A&AS, 123, 43. ...