activity
20062026
most citedHierarchical fragmentation and differential star formation in the Galactic "Snake": infrared dark cloud G11.11-0.12

264 citations · 3.8k across the 69 of their papers we have counts for

collaborators

70 papers

astro-ph.IM2026

Ushering in high angular resolution observatories in the far-infrared: The case for a double-Fourier interferometer

C. S. Benson, M. Bonato, T. A. Davis +14

A far-infrared (far-IR) interferometer from a space-based platform would bring about a transformational improvement in the spatial detail of astronomical observations that are inac…

astro-ph.GA2026

An ALMA study of hub-filament systems II.Quiescent filaments converging towards highly dynamic hubs

Michael Anderson, Nicolas Peretto, Sarah E. Ragan +7

Hub-filament systems are networks of converging interstellar filaments, often with active star formation at their centres, that may play an important role in high-mass star formati…

astro-ph.GA2026

MAJORS II: HCO+& HCN Abundances in W40

René Plume, David J. Eden, Malcolm J. Currie +34

We present observations of HCN and HCO J = in the central region of the W40 massive star forming region. The observations were taken as part of a p…

astro-ph.GA2024★ 20 cited

The dynamic centres of infrared-dark clouds and the formation of cores

Andrew J. Rigby, Nicolas Peretto, Michael Anderson +7

High-mass stars have an enormous influence on the evolution of the interstellar medium in galaxies, so it is important that we understand how they form. We examine the central clum…

astro-ph.GA2023

Density distributions, magnetic field structures and fragmentation in high-mass star formation

H. Beuther, C. Gieser, J. D. Soler +19

Methods: Observing the large pc-scale Stokes I mm dust continuum emission with the IRAM 30m telescope and the intermediate-scale (<0.1pc) polarized submm dust emission with the Sub…

astro-ph.GA2023★ 11 cited

Non-Equilibrium Abundances Treated Holistically (NEATH): the molecular composition of star-forming clouds

F. D. Priestley, P. C. Clark, S. C. O. Glover +4

Much of what we know about molecular clouds, and by extension star formation, comes from molecular line observations. Interpreting these correctly requires knowledge of the underly…