1.2k citations · 21k across the 225 of their papers we have counts for
53 papers · 1 filter
Highly-mass-loaded hot galactic winds are unstable to cool filament formation
Dustin D. Nguyen, Todd A. Thompson, Evan E. Schneider +1
When cool clouds are ram-pressure accelerated by a hot supersonic galactic wind, some of the clouds may be shredded by hydrodynamical instabilities and incorporated into the hot fl…
Dust Eddington Ratios for Star-Forming Galaxy Subregions
Ian Blackstone, Todd A. Thompson
Radiation pressure on dust is an important feedback process around star clusters and may eject gas from bright sub-regions in star-forming galaxies. The Eddington ratio has previou…
Cosmic-Ray Driven Galactic Winds from the Warm Interstellar Medium
Shaunak Modak, Eliot Quataert, Yan-Fei Jiang +1
We study the properties of cosmic-ray (CR) driven galactic winds from the warm interstellar medium using idealized spherically symmetric time-dependent simulations. The key ingredi…
Comparing the Locations of Supernovae to CO (2-1) Emission in their Host Galaxies
Ness Mayker Chen, Adam K. Leroy, Laura A. Lopez +19
We measure the molecular gas environment near recent ( yr old) supernovae (SNe) using or pc resolution CO (2-1) maps from the PHANGS-ALMA survey of nearb…
Dynamics of hot galactic winds launched from spherically-stratified starburst cores
Dustin D. Nguyen, Todd A. Thompson, Evan E. Schneider +2
The analytic galactic wind model derived by Chevalier and Clegg in 1985 (CC85) assumes energy and mass-injection within the starburst galaxy nucleus. However, th…
On Odd Radio Circles as Supernova Remnants
Sumit K. Sarbadhicary, Todd A. Thompson, Laura A. Lopez +1
The origin of arcmin-sized Odd Radio Circles (ORCs) found in modern all-sky radio surveys remain uncertain, with explanations ranging from starburst/AGN-driven shocks to supernova…