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20212026
most citedCosmic Ray Feedback on Bi-stable ISM Turbulence

6 citations · 13 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026

The Effects of Cosmic Ray Protons on Galactic Nonthermal Filaments

Mohan Richter-Addo, Roark Habegger, Ellen Zweibel +2

The Galactic Center (GC) contains a collection of filaments that are typically tens of parsecs in length, illuminated by synchrotron radiation from cosmic rays (CR). The origin of…

astro-ph.GA2025

The Impact of Cosmic Ray Transport on the -Ray Luminosity of Diffuse Gas

Roark Habegger, Mateusz Ruszkowski, Ellen G. Zweibel

Observations of -rays from diffuse gas provide the opportunity to study the distribution of high energy particles in different astrophysical environments. In the circumgalactic…

astro-ph.IM2024

A Co-Scaling Grid for Athena++ II: Magnetohydrodynamics

Fabian Heitsch, Roark Habegger

We extend the co-scaling formalism of Habegger & Heitsch (2021) implemented in Athena++ to magneto-hydrodynamics. The formalism relies on flow symmetries in astrophysical problems…

astro-ph.GA2024

Cosmic-Ray Feedback from Supernovae in a Parker-Unstable Medium

Roark Habegger, Ellen G. Zweibel

Supernova energy drives interstellar medium (ISM) turbulence and can help launch galactic winds. What difference does it make if of the energy is initially deposited into co…

astro-ph.HE2024★ 6 cited

Cosmic Ray Feedback on Bi-stable ISM Turbulence

Roark Habegger, Ka Wai Ho, Ka Ho Yuen +1

While cosmic rays are well coupled to a galaxy's interstellar medium (ISM) at scales of , adjusting stratification and driving outf…

astro-ph.HE2022★ 5 cited

The Impact of Cosmic Ray Injection on Magnetic Flux Tubes in a Galactic Disk

Roark Habegger, Ellen G. Zweibel, Sherry Wong

In galactic disks, the Parker instability results when non-thermal pressure support exceeds a certain threshold. The non-thermal pressures considered in the Parker instability are…

astro-ph.IM2021★ 2 cited

A Co-Scaling Grid for Athena++

Roark Habegger, Fabian Heitsch

We present a co-scaling grid formalism and its implementation in the magnetohydrodynamics code Athena++. The formalism relies on flow symmetries in astrophysical problems involving…