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19972026
most citedHow Do Galaxies Get Their Gas?

2.3k citations · 15.1k across the 152 of their papers we have counts for

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Showing 2018 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2018★ 58 cited

The Three Hundred Project: The evolution of galaxy cluster density profiles

Robert Mostoghiu, Alexander Knebe, Weiguang Cui +5

Recent numerical studies of the dark matter density profiles of massive galaxy clusters (M) show that their median radial mass density profile rem…

astro-ph.GA2018★ 24 cited

Dark Molecular Gas in Simulations of z~0 Disc Galaxies

Qi Li, Desika Narayanan, Romeel Dave +1

The mass of molecular clouds has traditionally been traced by the CO(J=1-0) rotational transition line. This said, CO is relatively easily photodissociated, and can also…

astro-ph.GA2018★ 1 cited

Science with an ngVLA: Imaging Cold Gas to 1 kpc Scales in High-Redshift Galaxies with the ngVLA

Caitlin M. Casey, Desika Narayanan, Chris Carilli +9

The next generation Very Large Array (ngVLA) will revolutionize our understanding of the distant Universe via the detection of cold molecular gas in the first galaxies. Its impact…

astro-ph.GA2018★ 231 cited

The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications

Weiguang Cui, Alexander Knebe, Gustavo Yepes +34

We introduce the THE THREE HUNDRED project, an endeavour to model 324 large galaxy clusters with full-physics hydrodynamical re-simulations. Here we present the data set and study…

astro-ph.GA2018★ 67 cited

Tracing Outflowing Metals in Simulations of Dwarf and Spiral Galaxies

Charlotte R. Christensen, Romeel Dave, Alyson Brooks +2

We analyze the metal accumulation in dwarf and spiral galaxies by following the history of metal enrichment and outflows in a suite of twenty high-resolution simulated galaxies. Th…

astro-ph.GA2018★ 126 cited

A Theory for the Variation of Dust Attenuation Laws in Galaxies

Desika Narayanan, Charlie Conroy, Romeel Dave +2

In this paper, we provide a physical model for the origin of variations in the shapes and bump strengths of dust attenuation laws in galaxies by combining a large suite of cosmolog…

astro-ph.GA2018★ 25 cited

On the Interpretation of Far-infrared Spectral Energy Distributions. I: The 850 m Molecular Mass Estimator

G. C. Privon, D. Narayanan, R. Davé

We use a suite of cosmological zoom galaxy formation simulations and dust radiative transfer calculations to explore the use of the monochromatic luminosity (L$_{\rm ν,850…