activity
20212026
most citedMagnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamics

28 citations · 79 across the 12 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

12 papers · 1 filter

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.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

A bottleneck for star formation: the importance of magnetic fields during the formation of cold gas in galaxies

Ryan McGuiness, Rowan J. Smith, David Whitworth

Using a high-resolution simulation of a dwarf galaxy, we quantify the energetic importance of magnetic fields within the different phases of its interstellar medium (ISM) on parsec…

astro-ph.GA2025★ 5 cited

The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies

Jonathan Petersson, Michaela Hirschmann, Robin G. Tress +6

Aims. We study the individual and cumulative impact of stellar feedback processes on massive black hole (MBH) growth in a simulated low-mass dwarf galaxy. Methods. A suite of high-…

astro-ph.GA2024

Do stars still form in molecular gas within CO-dark dwarf galaxies?

David J. Whitworth, Rowan J. Smith, Simon C. O. Glover +6

In the Milky Way and other main-sequence galaxies, stars form exclusively in molecular gas, which is traced by CO emission. However, low metallicity dwarf galaxies are often `CO-da…

astro-ph.GA2024

Filamentary Molecular Cloud Formation via Collision-induced Magnetic Reconnection in Cold Neutral Medium

Shuo Kong, Rowan J. Smith, David Whitworth +1

We have investigated the possibility of molecular cloud formation via the Collision-induced Magnetic Reconnection (CMR) mechanism of the cold neutral medium (CNM). Two atomic gas c…