activity
20002009
most citedBuilding Merger Trees from Cosmological N-body Simulations

254 citations · 674 across the 4 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2009254 cited

Building Merger Trees from Cosmological N-body Simulations

D. Tweed, J. Devriendt, J. Blaizot +2

Although a fair amount of work has been devoted to growing Monte-Carlo merger trees which resemble those built from an N-body simulation, comparatively little effort has been inves…

astro-ph2007196 cited

Cooling, Gravity and Geometry: Flow-driven Massive Core Formation

Fabian Heitsch, Lee Hartmann, Adrianne D. Slyz +2

We study numerically the formation of molecular clouds in large-scale colliding flows including self-gravity. The models emphasize the competition between the effects of gravity on…

astro-ph200612 cited

Cloud Dispersal in Turbulent Flows

F. Heitsch, A. D. Slyz, J. E. G. Devriendt +1

Cold clouds embedded in warm media are very common objects in astrophysics. Their disruption timescale depends strongly on the dynamical configuration. We discuss the evolution of…

astro-ph2006212 cited

The Birth of Molecular Clouds: Formation of Atomic Precursors in Colliding Flows

F. Heitsch, A. D. Slyz, J. E. G. Devriendt +2

Molecular Cloud Complexes (MCCs) are highly structured and ``turbulent''. Observational evidence suggests that MCCs are dynamically dominated systems, rather than quasi-equilibrium…

astro-ph2005

Formation of Structure in Molecular Clouds: A Case Study

F. Heitsch, A. Burkert, L. Hartmann +2

Molecular clouds (MCs) are highly structured and ``turbulent''. Colliding gas streams of atomic hydrogen have been suggested as a possible source of MCs, imprinting the filamentary…

astro-ph2004

Towards simulating star formation in the interstellar medium

A. Slyz, J. Devriendt, Greg Bryan +1

As a first step to a more complete understanding of the local physical processes which determine star formation rates (SFRs) in the interstellar medium (ISM), we have performed con…