activity
20182026
most citedCGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: dependence on redshift, halo mass and radius

31 citations · 41 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2026

Resolving galaxy formation in the early Universe with BonFIRE and CampFIRE

Jenna Samuel, Michael Boylan-Kolchin, Robert Feldmann +16

The abundance and rapid growth of galaxies at cosmic dawn revealed by the James Webb Space Telescope challenges models of galaxy formation, motivating new simulations to uncover th…

astro-ph.GA2026

From protogalaxy through thick and thin: Why did the Milky Way evolve in three kinematic phases?

Olti Myrtaj, James S. Bullock, Michael Boylan-Kolchin +9

APOGEE and Gaia data suggest the Milky Way's kinematic structure evolved through three distinct phases: a disordered protogalaxy, which ``spun up'' into a thick stellar disk, and t…

astro-ph.GA2026

Cold vs. Hot Gas Accretion and Angular Momentum in FIRE Simulations: From Halo to Galaxy Scales

Imran Sultan, Claude-André Faucher-Giguère, Jonathan Stern +1

We present a systematic study of gas accretion and angular momentum in the circumgalactic medium (CGM) using high-resolution FIRE cosmological simulations. Our analysis includes ha…

astro-ph.GA2026

Enhanced Multiphase Circumgalactic Medium and Gas Cycling in Galaxy Mergers

Maolan Yang, Suoqing Ji, Robert Feldmann +9

We investigate the impact of galaxy mergers on the circumgalactic medium (CGM) using the FIREbox cosmological hydrodynamic simulation. By comparing matched samples of merging and i…

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★ 1 cited

Project AMIGA: The Inner Circumgalactic Medium of Andromeda from Thick Disk to Halo

Nicolas Lehner, J. Christopher Howk, Lucy Collins +22

The inner circumgalactic medium (CGM) of galaxies, where disk and halo processes intersect, remains poorly characterized despite its critical role in regulating galaxy evolution. W…

astro-ph.GA2025

Turbulence-dominated CGM: the origin of UV absorbers with equivalent widths of Å

Aharon Kakoly, Jonathan Stern, Claude-André Faucher-Giguère +4

Theoretical arguments and observations suggest that in massive halos (), the circumgalactic medium (CGM) is dominated by a 'hot' phase with gas temperature near…

astro-ph.GA2025★ 6 cited

The Shape of FIREbox Galaxies and a Potential Tension with Low-mass Disks

Courtney Klein, Jenny D. Wang, Luke Xia +9

We study the intrinsic and observable shapes of approximately 700 star-forming galaxies with stellar masses of M from the FIREbox simulation at . We c…

astro-ph.GA2024

Cooling Flows as a Reference Solution for the Hot Circumgalactic Medium

Imran Sultan, Claude-André Faucher-Giguère, Jonathan Stern +3

The circumgalactic medium (CGM) in halos is dominated by a hot phase ( K). While many models exist for the hot gas structur…

astro-ph.GA2024

Comparison of Models for the Warm-Hot Circumgalactic Medium around Milky Way-like Galaxies

Priyanka Singh, Erwin T. Lau, Yakov Faerman +2

A systematic comparison of the models of the circumgalactic medium (CGM) and their observables is crucial to understanding the predictive power of the models and constraining physi…

astro-ph.GA2024

X-ray signatures of galactic outflows into the circumgalactic medium

Ranita Jana, Kartick C. Sarkar, Jonathan Stern +1

We present a set of controlled hydrodynamical simulations to study the effects of strong galactic outflows on the density and temperature structures, and associated X-ray signature…

astro-ph.GA2024

Ne VIII in the warm-hot circumgalactic medium of FIRE simulations and in observations

Nastasha A. Wijers, Claude-André Faucher-Giguère, Jonathan Stern +2

The properties of warm-hot gas around galaxies can be studied with absorption lines from highly ionized metals. We predict Ne VIII column densities from cosmological z…

astro-ph.GA2018★ 31 cited

CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: dependence on redshift, halo mass and radius

S. Roca-Fàbrega, A. Dekel, Y. Faerman +8

We study the components of cool and warm/hot gas in the circumgalactic medium (CGM) of simulated galaxies and address the relative production of OVI by photoionization versus colli…