activity
20062026
most citedComparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcing

847 citations · 2.4k across the 23 of their papers we have counts for

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Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2026

Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes. III. Mass Distribution of Hierarchical Mergers

Katherine L. Gonglewski, Amy Secunda, Mordecai-Mark Mac Low +3

Active galactic nucleus (AGN) disks are a promising location for the formation of binary black holes (BBHs) that will merge on relatively short timescales and be detected by LIGO-V…

astro-ph.GA2026

Centrally concentrated star formation in young clusters II: Jet feedback

Adilkhan Assilkhan, Sabrina M. Appel, Bekdaulet Shukirgaliyev +5

Protostellar jets are one of the earliest forms of stellar feedback, but their impact on star formation and cluster assembly in centrally concentrated molecular clouds remains poor…

astro-ph.GA2026

On the relation between magnetic field strength and gas density in the interstellar medium. II. Density uncertainties and diffuse gas constraints

David Whitworth, Amit Seta, Ralph E. Pudritz +4

The relationship between magnetic field strength and gas density is essential to understand the interstellar medium and star formation. Zeeman measurements in dense atomic and mole…

astro-ph.GA2026

Evolution of fractality in centrally concentrated young clusters

Almat Akhmetali, Adilkhan Assilkhan, Mordecai-Mark Mac Low +6

We investigate the structural evolution of young star clusters forming within centrally concentrated molecular clouds. Our simulations use the Torch framework, which integrates the…

astro-ph.GA2025

How is cold, star-forming gas in galaxies affected by magnetic fields?

Kamran R. J. Bogue, Rowan J. Smith, Robin G. Tress +9

Numerical simulations provide a unique opportunity to improve our understanding of the role of magnetic fields in the interstellar medium of galaxies and in star formation. However…

astro-ph.GA2025

EDGE-INFERNO: How chemical enrichment assumptions impact the individual stars of a simulated ultra-faint dwarf galaxy

Eric P. Andersson, Martin P. Rey, Robert M. Yates +6

The chemical abundances of stars in galaxies are a fossil record of the star formation and stellar evolution processes that regulate galaxy formation, including the stellar initial…