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19962026
most citedHot One-Temperature Accretion Flows Around Black Holes

87 citations · 268 across the 23 of their papers we have counts for

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Showing 2025Show all

6 papers · 1 filter

astro-ph.HE2025

Estimation of Magnetic Fields from Synchrotron Emission: Numerical Tests

Nora B. Linzer, Lucia Armillotta, Eve C. Ostriker +1

We use models of spectrally resolved cosmic ray (CR) transport in TIGRESS MHD simulations of the local ISM to produce synthetic synchrotron emission and to test, on scales from a f…

astro-ph.HE2025★ 1 cited

Cosmic Ray Magnetohydrodynamics: A New Two-Moment Framework with Numerical Implementation

Xihui Zhao, Xue-Ning Bai, Eve C. Ostriker

Cosmic rays (CRs) play a pivotal role in various astrophysical systems, delivering feedback over a broad range of scales. However, modeling CR transport remains challenging due to…

astro-ph.HE2025

Modeling Cosmic Ray Electron Spectra and Synchrotron Emission in the Multiphase ISM

Nora B. Linzer, Lucia Armillotta, Eve C. Ostriker +1

We model the transport and spectral evolution of 1-100 GeV cosmic ray (CR) electrons (CREs) in TIGRESS MHD simulations of the magnetized, multiphase interstellar medium. We post-pr…

astro-ph.HE2025

Energy-Dependent Transport of Cosmic Rays in the Multiphase, Dynamic Interstellar Medium

Lucia Armillotta, Eve C. Ostriker, Nora B. Linzer

We investigate the transport of spectrally resolved cosmic ray (CR) protons with kinetic energies between GeV within the dynamic, multiphase interstellar medium (ISM), usin…

astro-ph.GA2025★ 5 cited

Modeling the Mass Distribution and Gravitational Potential of Nearby Disk Galaxies: Implications for the ISM Dynamical Equilibrium

Vivek Vijayakumar, Jiayi Sun, Eve C. Ostriker +5

We characterize stellar, gas, and dark matter mass distributions for 17 nearby massive disk galaxies from the PHANGS sample. This allows us to compute the gravitational potential t…

astro-ph.GA2025

Characterizing Density and Gravitational Potential Fluctuations of the Interstellar Medium

Shaunak Modak, Eve C. Ostriker, Chris Hamilton +1

Substructure in the interstellar medium (ISM) is crucial for establishing the correlation between star formation and feedback and has the capacity to significantly perturb stellar…