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From the 1 of 9 linked papers with an AI index.

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9 papers

astro-ph.GA2026

Measuring Simulated Circumgalactic Medium Turbulence with Emission-Weighted Projected Velocity Structure Functions in FOGGIE

Helena Bouchereau, Cassandra Lochhaas, Jake S. Bennett +1

The spatially-resolved kinematics of line emission from the circumgalactic medium (CGM) of a galaxy can contain information about the CGM turbulence, which may play an important ro…

astro-ph.GA2026

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H nebulae at

Lucas Tortora, Tiago Costa, Debora Sijacki +1

The discovery of gargantuan black holes with masses exceeding a billion solar masses at suggests rapid black hole growth and significant energy input into their host ga…

astro-ph.GA2026

The birth of the intracluster medium: the evolution of multiphase gas and Lyman- haloes in a simulated protocluster

Jake S. Bennett, Aaron Smith, Fabrizio Arrigoni-Battaia +3

The paper uses a high‑resolution cosmological zoom‑in simulation of a massive protocluster to study how multiphase gas and Lyman‑α/ H‑α haloes evolve from redshift ~4.4 to 2.7, hig…

astro-ph.GA2026

Too many protoclusters? Reconciling the overabundance of cluster progenitors within the first billion years of the Universe

Callum Witten, Jake S. Bennett, Pascal A. Oesch +8

JWST has revealed an overabundance of apparent (`Coma'-like) cluster progenitors at that is two (300) times in excess of, and in () tension with, the numb…

astro-ph.GA2026

ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations

James M. Sullivan, Greg L. Bryan, Matthew C. Smith +6

AGN feedback is a key piece of galaxy evolution but is difficult to model due to its high specific energies, multiphase nature, and limited simulation resolutions. Arkenstone is a…

astro-ph.GA2025

MISTRAL: a model for AGN winds from radiatively efficient accretion in cosmological simulations

Marion Farcy, Michaela Hirschmann, Rachel S. Somerville +11

Feedback from active galactic nuclei (AGN) is crucial for regulating galaxy evolution. Motivated by observations of broad absorption line winds from rapidly accreting supermassive…