2 citations · 3 across the 3 of their papers we have counts for
3 papers
astro-ph2005
The colliding-wind binary WR140: the particle acceleration laboratory
S. M. Dougherty, J. M. Pittard
WR+O star binary systems exhibit synchrotron emission arising from relativistic electrons accelerated where the wind of the WR star and that of its massive binary companion collide…
astro-ph2005★ 2 cited
Radio emission from Colliding-Wind Binaries: Observations and Models
S. M. Dougherty, J. M. Pittard, E. P. O'Connor
We have developed radiative transfer models of the radio emission from colliding-wind binaries (CWB) based on a hydrodynamical treatment of the wind-collision region (WCR). The arc…
astro-ph2005★ 1 cited
The Colliding Winds of WR146: Seeing the Works
E. P. O'Connor, S. M. Dougherty, J. M. Pittard +1
WR146 is a WC6+O8 colliding-wind binary (CWB) system with thermal emission from the stellar winds of the two stars, and bright non-thermal emission from the wind-collision region (…