261 citations · 1.7k across the 44 of their papers we have counts for
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The Large Adaptive Reflector concept
S. M. Dougherty, P. E. Dewdney, A. Gray +1
Cost effective, new antenna technology is required to build the large collecting area being planned for the next generation of radio telescopes. The Large Adaptive Reflector (LAR)…
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…
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…
Radio emission models of Colliding-Wind Binary Systems - Inclusion of IC cooling
J. M. Pittard, S. M. Dougherty, R. F. Coker +2
Radio emission models of colliding wind binaries (CWBs) have been discussed by Dougherty et al. (2003). We extend these models by considering the temporal and spatial evolution of…
Non-thermal X-ray and Gamma-ray Emission from the Colliding Wind Binary WR140
J. M. Pittard, S. M. Dougherty
WR140 is the archetype long-period colliding wind binary (CWB) system, and is well known for dramatic variations in its synchrotron emission during its 7.9-yr, highly eccentric orb…
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 (…