most citedArkenstone -- II. A model for unresolved cool clouds entrained in galactic winds in cosmological simulations

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astro-ph.GA2025

The MandelZoom project II: the impact of stellar feedback on black hole accretion through an -disc in dwarf galaxies with a resolved interstellar medium

Eun-jin Shin, Matthew C. Smith, Debora Sijacki +2

We present a suite of high-resolution simulations to study how different stellar feedback channels regulate the growth of central intermediate-mass black holes (IMBHs) in dwarf gal…

astro-ph.GA2025

The MandelZoom project I: modelling black hole accretion through an -disc in dwarf galaxies with a resolved interstellar medium

Eun-jin Shin, Debora Sijacki, Matthew C. Smith +2

While mounting observational evidence suggests that intermediate mass black holes (IMBHs) may be important in shaping the properties of dwarf galaxies both at high redshifts and in…

astro-ph.GA2025

Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation

Jan D. Burger, Volker Springel, Eve C. Ostriker +11

Modern high-resolution simulations of the interstellar medium (ISM) have shown that key factors in governing star formation are the competing influences of radiative dissipation, p…

astro-ph.GA2024

Prevention is better than cure? Feedback from high specific energy winds in cosmological simulations with Arkenstone

Jake S. Bennett, Matthew C. Smith, Drummond B. Fielding +6

We deploy the new Arkenstone galactic wind model in cosmological simulations for the first time, allowing us to robustly resolve the evolution and impact of high specific energy wi…

astro-ph.GA2024

Towards Implementation of the Pressure-Regulated, Feedback-Modulated Model of Star Formation in Cosmological Simulations: Methods and Application to TNG

Sultan Hassan, Eve C. Ostriker, Chang-Goo Kim +12

Traditional star formation subgrid models implemented in cosmological galaxy formation simulations, such as that of Springel & Hernquist (2003, hereafter SH03), employ adjustable p…

astro-ph.GA20241 cited

Arkenstone -- II. A model for unresolved cool clouds entrained in galactic winds in cosmological simulations

Matthew C. Smith, Drummond B. Fielding, Greg L. Bryan +4

Arkenstone is a new scheme that allows multiphase, stellar feedback-driven winds to be included in coarse resolution cosmological simulations. The evolution of galactic winds and t…