activity
20152024
most citedProperties of Hi-GAL clumps in the inner Galaxy]{The Hi-GAL compact source catalogue. I. The physical properties of the clumps in the inner Galaxy ()

201 citations · 526 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2024★ 1 cited

The SARAO MeerKAT Galactic Plane Survey filamentary source catalogue

Gwenllian M. Williams, Mark A. Thompson, Mubela Mutale +11

We present a catalogue of filamentary structures identified in the SARAO (South African Radio Astronomy Observatory) MeerKAT 1.3 GHz Galactic Plane Survey (SMGPS). We extract 933 f…

astro-ph.GA2023

Can massive stars form in low mass clouds?

Jamie D. Smith, Sarah E. Jaffa, Martin G. H. Krause

The conditions required for massive star formation are debated, particularly whether massive stars must form in conjunction with massive clusters. Some authors have advanced the vi…

cs.HC2022

Gather -- a better way to codehack online

Rika Kobayashi, Sarah Jaffa, Jiachen Dong +3

A virtual hands-on computer laboratory has been designed within the Gather online meeting platform. Gather's features such as spatial audio, private spaces and interactable objects…

astro-ph.GA2022★ 10 cited

RJ-plots: An improved method to classify structures objectively

Seamus D. Clarke, Sarah E. Jaffa, Anthony P. Whitworth

The interstellar medium is highly structured, presenting a range of morphologies across spatial scales. The large data sets resulting from observational surveys and state-of-the-ar…

astro-ph.GA2022★ 4 cited

Star Cluster Formation in Clouds with Externally Driven Turbulence

Jamie D. Smith, James E. Dale, Sarah E. Jaffa +1

Star clusters are known to be formed in turbulent molecular clouds. How turbulence is driven in molecular clouds and what effect this has on star formation is still unclear. We com…

astro-ph.GA2021

Grouped star formation: converting sink particles to stars in hydrodynamical simulations

K. Y. Liow, S. Rieder, C. L. Dobbs +1

Modelling star formation and resolving individual stars in numerical simulations of molecular clouds and galaxies is highly challenging. Simulations on very small scales can be suf…