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most citedThe stellar mass spectrum from non-isothermal gravoturbulent fragmentation

313 citations · 2.7k across the 44 of their papers we have counts for

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astro-ph2004★ 313 cited

The stellar mass spectrum from non-isothermal gravoturbulent fragmentation

Anne-Katharina Jappsen, Ralf S. Klessen, Richard B. Larson +2

Identifying the processes that determine the initial mass function of stars (IMF) is a fundamental problem in star formation theory. One of the major uncertainties is the exact che…

astro-ph2004★ 5 cited

Initial Ionization of Compressible Turbulence

Yuexing Li, Mordecai-Mark Mac Low, Tom Abel

We study the effects of the initial conditions of turbulent molecular clouds on the ionization structure in newly formed H_{ii} regions, using three-dimensional, photon-conserving…

astro-ph2004★ 71 cited

Formation of Globular Clusters in Galaxy Mergers

Yuexing Li, Mordecai-Mark Mac Low, Ralf S. Klessen

We present a high-resolution simulation of globular cluster formation in a galaxy merger. For the first time in such a simulation, individual star clusters are directly identified…

astro-ph2004★ 89 cited

Control of Star Formation in Galaxies by Gravitational Instability

Yuexing Li, Mordecai-Mark Mac Low, Ralf S. Klessen

We study gravitational instability and consequent star formation in a wide range of isolated disk galaxies, using three-dimensional, smoothed particle hydrodynamics simulations at…

astro-ph2004★ 3 cited

Gravoturbulent Star Cluster Formation

Ralf S. Klessen, Javier Ballesteros-Paredes, Yuexing Li +1

Stars form by gravoturbulent fragmentation of interstellar gas clouds. The supersonic turbulence ubiquitously observed in Galactic molecular gas generates strong density fluctuatio…