activity
20152025
most citedFilamentary fragmentation in a turbulent medium

113 citations · 844 across the 31 of their papers we have counts for

collaborators
Showing 2022Show all

6 papers · 1 filter

astro-ph.GA2022★ 8 cited

A Herschel study of G214.5-1.8: a young, cold and quiescent giant molecular filament on the shell of a HI superbubble

S. D. Clarke, A. Sanchez-Monge, G. M. Williams +3

We present an analysis of the outer Galaxy giant molecular filament (GMF) G214.5-1.8 (G214.5) using Herschel data. We find that G214.5 has a mass of 16,000 M, yet…

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★ 55 cited

Understanding star formation in molecular clouds IV. Column density PDFs from quiescent to massive molecular clouds

N. Schneider, V. Ossenkopf-Okada, S. Clarke +26

We present N-PDFs of 29 Galactic regions obtained from Herschel imaging at high angular resolution, covering diffuse and quiescent clouds, and those showing low-, intermediate-, an…

astro-ph.GA2022

From Bubbles and Filaments to Cores and Disks: Gas Gathering and Growth of Structure Leading to the Formation of Stellar Systems

Jaime E. Pineda, Doris Arzoumanian, Philippe André +8

The study of the development of structures on multiple scales in the cold interstellar medium has experienced rapid expansion in the past decade, on both the observational and the…

astro-ph.GA2022★ 4 cited

SILCC-Zoom: the dynamic balance in molecular cloud substructures

S. Ganguly, S. Walch, S. D. Clarke +1

How molecular clouds fragment and create the dense structures which go on to form stars is an open question. We investigate the relative importance of different energy terms (kinet…

astro-ph.SR2022★ 5 cited

Protostellar Outflows: a window to the past

P. F. Rohde, S. Walch, D. Seifried +2

During the early phases of low-mass star formation, episodic accretion causes the ejection of high-velocity outflow bullets, which carry a fossil record of the driving protostar's…