activity
20022025
most citedThe SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM

367 citations · 6.4k across the 103 of their papers we have counts for

collaborators
Showing 2011Show all

5 papers · 1 filter

astro-ph.GA2011★ 55 cited

Comparing simulations of ionisation triggered star formation and observations in RCW 120

S. Walch, A. Whitworth, T. Bisbas +2

Massive clumps within the swept-up shells of bubbles, like that surrounding the galactic HII region RCW 120, have been interpreted in terms of the Collect and Collapse (C&C) mechan…

astro-ph.GA2011★ 45 cited

The influence of the turbulent perturbation scale on prestellar core fragmentation and disk formation

S. Walch, A. P. Whitworth, P. Girichidis

The collapse of weakly turbulent prestellar cores is a critical stage in the process of star formation. Being highly non-linear and stochastic, the outcome of collapse can only be…

astro-ph.SR2011★ 132 cited

Radiation driven implosion and triggered star formation

Thomas G. Bisbas, Richard Wunsch, Anthony P. Whitworth +2

We present simulations of initially stable isothermal clouds exposed to ionising radiation from a discrete external source, and identify the conditions that lead to radiatively dri…

astro-ph.GA2011★ 31 cited

Flow-Driven Cloud Formation and Fragmentation: Results From Eulerian and Lagrangian Simulations

Fabian Heitsch, Thorsten Naab, Stefanie Walch

The fragmentation of shocked flows in a thermally bistable medium provides a natural mechanism to form turbulent cold clouds as precursors to molecular clouds. Yet because of the l…

astro-ph.GA2011★ 33 cited

The turbulent fragmentation of the interstellar medium: The impact of metallicity on global star formation

S. Walch, R. Wuensch, A. Burkert +2

We study the influence of gas metallicity, turbulence, and non-equilibrium chemistry on the evolution of the two-phase interstellar medium (warm and cold atomic phases), and thereb…