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

collaborators

22 papers

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.IM2026

Iterative Poisson Solvers for Self-gravity with the GPU Code Astaroth

Ruben Krasnopolsky, Touko Puro, Wei-Wen Li +5

We present the development and benchmarking of Poisson solvers for graphics processing units (GPUs). Implemented in the Astaroth platform, the solvers feature high computational ef…

astro-ph.EP2026

Active Galactic Nucleus Tori: Potential Birthplace to Millions of Planets

Bhupendra Mishra, Wladimir Lyra, Barry McKernan +3

The outer regions of AGN disks have temperatures similar to those of circumstellar disks, permitting dust condensation. Therefore, planet formation and growth could be active in th…

astro-ph.HE2026

AGN Disks as Supernova Mufflers I: 3D Local Hydrodynamic Models

Harrison E. Cook, Wladimir Lyra, Mordecai-Mark Mac Low +2

Supernova (SN) shocks that originate from stars on orbits embedded in dense active galactic nuclei (AGN) accretion disks evolve differently from those that occur in the interstella…

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…