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Dynamics of Dusty Radiation Pressure Driven Shells and Clouds: Fast Outflows from Galaxies, Star Clusters, Massive Stars, and AGN
Todd A. Thompson, Andrew C. Fabian, Eliot Quataert +1
It is typically assumed that radiation pressure driven winds are accelerated to an asymptotic velocity of V ~ v_esc, where v_esc is the escape velocity from the central source. We…
A Solar Mass Flow of Molecular Gas in the Abell 1835 Brightest Cluster Galaxy
B. R. McNamara, H. R. Russell, P. E. J. Nulsen +17
We report ALMA Early Science observations of the Abell 1835 brightest cluster galaxy (BCG) in the CO (3-2) and CO (1-0) emission lines. We detect of m…
Radiation Feedback in ULIRGS: Are Photons Movers and Shakers?
Shane W. Davis, Yan-Fei Jiang, James M. Stone +1
We use our variable Eddington tensor (VET) radiation hydrodynamics code to perform two-dimensional simulations to study the impact of radiation forces on atmospheres composed of du…