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Presentation #204.08 in the session “Massive Stars in Colliding Wind Binaries”.
Radio emission is an important component in understanding how colliding wind binaries (CWBs) work. In this talk, I will quickly review the radio emission processes in CWBs (both thermal and non-thermal processes) and then introduce some new results on the extremely variable radio emission from the WR140 system, with data from both the GMRT and EAVN radio telescopes.