activity
19962026
most citedHot One-Temperature Accretion Flows Around Black Holes

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

collaborators

23 papers

astro-ph.GA2026

A Multiwavelength Inventory for the Local Group L-band Survey I: Atlas and Radial Profiles of Local Group Galaxies

Cosima Eibensteiner, Adam K. Leroy, Jiayi Sun +21

Resolving atomic gas at pc physical resolution is currently feasible only for the very nearest galaxies. We combine 120 pc resolution HI data using the Karl G. Jansky…

astro-ph.GA2026

Pressure-regulated feedback-modulated star formation as a subgrid model for galaxy formation simulations

Sarah M. R. Jeffreson, Eve C. Ostriker, Chang-Goo Kim +1

We present a new subgrid model for interstellar gas evolution in cosmological simulations of galaxy formation, based on the pressure-regulated, feedback-modulated (PRFM) theory of…

astro-ph.GA2026

Learning the Universe with PRFM-vol: Introducing a new subgrid model for star formation in cosmological simulations

Jan D. Burger, Volker Springel, Eve C. Ostriker +7

We introduce PRFM-vol, a new subgrid model for star formation in cosmological simulations that aims to increase the physical realism of cosmological simulations by leveraging resul…

astro-ph.GA2026

Cosmic Ray Feedback in Galactic Disks: Star Formation, Cosmic Ray Transport, and Multiphase Outflows in TIGRESS++ Simulations

Chang-Goo Kim, Lucia Armillotta, Eve C. Ostriker +5

We present new simulations of local star-forming disks that self-consistently evolve cosmic rays (CRs) and multiphase gas using TIGRESS++. To isolate the role of CRs, we conduct pa…

astro-ph.GA2026

Interstellar Medium-Driven Orbital Transport -- I. Radial Heating and Migration

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

Interstellar medium (ISM) structures gravitationally perturb stellar orbits in galactic disks, driving orbital heating and migration. However, studies of these transport processes…

astro-ph.GA2026

Stellar associations powering HII regions $\unicode{x2013}$ II. Escape fraction of ionizing photons

Fabian Scheuermann, Kathryn Kreckel, Jia Wei Teh +27

Newly formed stars have a profound impact on their environment by depositing energy and momentum into the surrounding gas. However, only a fraction of the stellar feedback is retai…

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…

astro-ph.GA2024

Polycyclic Aromatic Hydrocarbon and CO(2-1) Emission at 50-150 pc Scales in 70 Nearby Galaxies

Ryan Chown, Adam K. Leroy, Karin Sandstrom +44

Combining Atacama Large Millimeter/sub-millimeter Array CO(2-1) mapping and JWST near- and mid-infrared imaging, we characterize the relationship between CO(2-1) and polycyclic aro…

astro-ph.GA2024★ 19 cited

PHANGS-MeerKAT and MHONGOOSE HI observations of nearby spiral galaxies: physical drivers of the molecular gas fraction,

Cosima Eibensteiner, Jiayi Sun, Frank Bigiel +36

The molecular-to-atomic gas ratio is crucial to the evolution of the interstellar medium in galaxies. We investigate the balance between the atomic () and molecular gas…

astro-ph.GA2024

JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbon Emission at the Base of the M 82 Galactic Wind

Alberto D. Bolatto, Rebecca C. Levy, Elizabeth Tarantino +37

We present new observations of the central 1 kpc of the M 82 starburst obtained with the James Webb Space Telescope (JWST) near-infrared camera (NIRCam) instrument at a resolution…

astro-ph.GA2024

Hidden Gems on a Ring: Infant Massive Clusters and Their Formation Timeline Unveiled by ALMA, HST, and JWST in NGC 3351

Jiayi Sun, Hao He, Kyle Batschkun +38

We study young massive clusters (YMCs) in their embedded "infant" phase with ALMA, HST, and JWST observations targeting the central starburst ring in NGC…

astro-ph.GA2023

Dynamics in Star-forming Cores (DiSCo): Project Overview and the First Look toward the B1 and NGC 1333 Regions in Perseus

Che-Yu Chen, Rachel Friesen, Jialu Li +13

The internal velocity structure within dense gaseous cores plays a crucial role in providing the initial conditions for star formation in molecular clouds. However, the kinematic p…

astro-ph.GA2023

A Two-Component Probability Distribution Function Describes the mid-IR Emission from the Disks of Star-Forming Galaxies

Debosmita Pathak, Adam K. Leroy, Todd A. Thompson +28

High-resolution JWST-MIRI images of nearby spiral galaxies reveal emission with complex substructures that trace dust heated both by massive young stars and the diffuse interstella…

astro-ph.GA2023

Star Formation Efficiency in Nearby Galaxies Revealed with a New CO-to-H2 Conversion Factor Prescription

Yu-Hsuan Teng, I-Da Chiang, Karin M. Sandstrom +24

Determining how galactic environment, especially the high gas densities and complex dynamics in bar-fed galaxy centers, alters the star formation efficiency (SFE) of molecular gas…

astro-ph.GA2021★ 48 cited

EDGE-CALIFA survey: Self-regulation of Star formation at kpc scales

J. K. Barrera-Ballesteros, S. F. Sánchez, T. Heckman +11

We present the relation between the star formation rate surface density, , and the hydrostatic mid-plane pressure, P, for 4260 star-forming regions of kpc si…

astro-ph.GA2017★ 61 cited

The EDGE-CALIFA survey: the influence of galactic rotation on the molecular depletion time across the Hubble sequence

D. Colombo, V. Kalinova, D. Utomo +15

We present a kpc-scale analysis of the relationship between the molecular depletion time () and the orbital time () across the field of…

astro-ph.GA2014★ 47 cited

CARMA Large Area Star Formation Survey: Project Overview with Analysis of Dense Gas Structure and Kinematics in Barnard 1

S. Storm, L. G. Mundy, M. Fernández-López +22

We present details of the CARMA Large Area Star Formation Survey (CLASSy), while focusing on observations of Barnard 1. CLASSy is a CARMA Key Project that spectrally imaged N2H+, H…

astro-ph1996★ 87 cited

Hot One-Temperature Accretion Flows Around Black Holes

A. A. Esin, R. Narayan, E. Ostriker +1

We describe hot, optically-thin solutions for one-temperature accretion disks around black holes. We include cooling by synchrotron, bremsstrahlung, and Comptonization. Our solutio…