activity
20122026
most citedThe Impact of Star Formation Feedback on the Circumgalactic Medium

177 citations · 2.8k across the 85 of their papers we have counts for

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Showing 2025Show all

9 papers · 1 filter

astro-ph.GA2025★ 1 cited

Hot accretion onto spiral galaxies: the origin of extended and warped HI discs

Sriram Sankar, Jonathan Stern, Chris Power +6

Gas accretion, hot ( K) atmospheres, and a tilt between the rotation axes of the disc and the atmosphere are all common predictions of standard galaxy evolution theory f…

astro-ph.GA2025★ 3 cited

Accretion-Driven Turbulence in the Circumgalactic Medium

Roy Goldner, Jonathan Stern, Drummond Fielding +3

Simulations suggest that turbulence is ubiquitous in the circumgalactic medium (CGM), though the source and properties of CGM turbulence is uncertain. Using analytic considerations…

astro-ph.GA2025

Modeling Emission-Line Surface Brightness in a Multiphase Galactic Wind: An O VI Case Study

Zirui Chen, Zixuan Peng, Kate H. R. Rubin +6

We present a fast and robust analytic framework for predicting surface brightness (SB) of emission lines in galactic winds as a function of radius up to kpc out in the c…

astro-ph.HE2025

Self-Similar Cosmic-Ray Transport in High-Resolution Magnetohydrodynamic Turbulence

Philipp Kempski, Drummond B. Fielding, Eliot Quataert +5

We study the propagation of cosmic rays (CRs) through a simulation of magnetohydrodynamic (MHD) turbulence at unprecedented resolution of . We drive turbulence that is…

astro-ph.GA2025

Simulating High-Velocity Clouds in the Observational Plane: An Initial Study with the Smith Cloud

Lori E. Porter, Matthew Abruzzo, Greg L. Bryan +3

High-velocity clouds (HVCs) may fuel future star formation in the Milky Way, but they must first survive their passage through the hot halo. While recent work has improved our unde…

astro-ph.GA2025

Neutral gas phase distribution from HI morphology: phase separation with scattering spectra and variational autoencoders

Minjie Lei, S. E. Clark, Rudy Morel +4

Unraveling the multi-phase structure of the diffuse interstellar medium (ISM) as traced by neutral hydrogen (HI) is essential to understanding the lifecycle of the Milky Way. Howev…