53 citations · 378 across the 26 of their papers we have counts for
26 papers
Numerical Modeling of Galactic Superwinds with Time-evolving Stellar Feedback
A. Danehkar, M. S. Oey, W. J. Gray
Mass-loss and radiation feedback from evolving massive stars produce galactic-scale superwinds, sometimes surrounded by pressure-driven bubbles. Using the time-dependent stellar po…
Hydrodynamic Simulations and Time-dependent Photoionization Modeling of Starburst-driven Superwinds
A. Danehkar, M. S. Oey, W. J. Gray
Thermal energies deposited by OB stellar clusters in starburst galaxies lead to the formation of galactic superwinds. Multi-wavelength observations of starburst-driven superwinds p…
Catastrophic Cooling in Superwinds. III. Non-equilibrium Photoionization
A. Danehkar, M. S. Oey, W. J. Gray
Observations of some starburst-driven galactic superwinds suggest that strong radiative cooling could play a key role in the nature of feedback and the formation of stars and molec…
Modeling Photoionized Turbulent Material in the Circumgalactic Medium III: Effects of Co-rotation and Magnetic Fields
Edward Buie, Evan Scannapieco, G. Mark Voit
Absorption-line measurements of the circumgalactic medium (CGM) display a highly non-uniform distribution of lower ionization state species accompanied by more widespread higher io…
Experimental observations of detached bow shock formation in the interaction of a laser-produced plasma with a magnetized obstacle
Joseph M. Levesque, Andy S. Liao, Patrick Hartigan +14
The magnetic field produced by planets with active dynamos, like the Earth, can exert sufficient pressure to oppose supersonic stellar wind plasmas, leading to the formation of a s…
Non-equilibrium Photoionization and Hydrodynamic Simulations of Starburst-driven Outflows
A. Danehkar, M. S. Oey, W. J. Gray
Starburst-driven galactic outflows in star-forming galaxies have been observed to contain complex thermal structures and emission line features that are difficult to explain by adi…