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20022026
most citedHow Do Galaxies Get Their Gas?

2.3k citations · 22.1k across the 139 of their papers we have counts for

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Showing 2023Show all

6 papers · 1 filter

astro-ph.GA2023★ 1 cited

Observational Signatures of AGN Feedback in the Morphology and the Ionization States of Milky Way-like Galaxies

Nadia Qutob, Razieh Emami, Kung-Yi Su +24

We make an in-depth analysis of different AGN jet models' signatures, inducing quiescence in galaxies with a halo mass of . Three jet models, including cosmic ray-…

astro-ph.GA2023★ 2 cited

Unraveling Jet Quenching Criteria Across L* Galaxies and Massive Cluster Ellipticals

Kung-Yi Su, Greg L. Bryan, Christopher C. Hayward +8

In the absence of supplementary heat, the radiative cooling of halo gas around massive galaxies (Milky Way mass and above) leads to an excess of cold gas or stars beyond observed l…

astro-ph.GA2023★ 2 cited

Synchrotron Signatures of Cosmic Ray Transport Physics in Galaxies

Sam B. Ponnada, Iryna S. Butsky, Raphael Skalidis +7

Cosmic rays (CRs) may drive outflows and alter the phase structure of the circumgalactic medium, with potentially important implications on galaxy formation. However, these effects…

astro-ph.GA2023★ 50 cited

FORGE'd in FIRE: Resolving the End of Star Formation and Structure of AGN Accretion Disks from Cosmological Initial Conditions

Philip F. Hopkins, Michael Y. Grudic, Kung-Yi Su +8

It has recently become possible to zoom-in from cosmological to sub-pc scales in galaxy simulations to follow accretion onto supermassive black holes (SMBHs). However, at some poin…

astro-ph.GA2023★ 19 cited

Synchrotron Emission on FIRE: Equipartition Estimators of Magnetic Fields in Simulated Galaxies with Spectrally-Resolved Cosmic Rays

Sam B. Ponnada, Georgia V. Panopoulou, Iryna S. Butsky +7

Synchrotron emission is one of few observable tracers of galactic magnetic fields (\textbf{B}) and cosmic rays (CRs). Much of our understanding of \textbf{B} in galaxies comes from…

astro-ph.GA2023★ 95 cited

What Causes The Formation of Disks and End of Bursty Star Formation?

Philip F. Hopkins, Alexander B. Gurvich, Xuejian Shen +17

As they grow, galaxies can transition from irregular/spheroidal with 'bursty' star formation histories (SFHs), to disky with smooth SFHs. But even in simulations, the direct physic…