activity
19962009
most citedNew electron source concept for single-shot sub-100 fs electron diffraction in the 100 keV range

227 citations · 1.2k across the 37 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

12 papers · 2 filters

astro-ph2005

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)…

astro-ph2005

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

C^2-Ray: A new method for photon-conserving transport of ionizing radiation

Garrelt Mellema, Ilian T. Iliev, Marcelo A. Alvarez +1

We present a new numerical method for calculating the transfer of ionizing radiation, called C^2-Ray=Conservative, Causal Ray-tracing method. The method is explicitly photon-conser…

astro-ph2005

Completing the Census of (Bright) Variable Stars in Galactic Globular Clusters

M. Catelan, H. A. Smith, B. J. Pritzl +15

We present a long-term project aimed at completing the census of (bright) variable stars in Galactic globular clusters. While our main aim is to obtain a reliable assessment of the…

astro-ph2005

Radial transport of dust in spiral galaxies

E. I. Vorobyov, Yu. A. Shchekinov

Motivated by recent observations which detect dust at large galactocentric distances in the disks of spiral galaxies, we propose a mechanism of outward radial transport of dust by…

astro-ph2005

Controlling the collimation and rotation of hydromagnetic disk winds

Ralph E. Pudritz, Conrad Rogers, Rachid Ouyed

(Abriged) We present a comprehensive set of axisymmetric, time-dependent simulations of jets from Keplerian disks whose mass loading as a function of disk radius is systematically…