activity
20072009
most citedStar formation at very low metallicity. I: Chemistry and cooling at low densities

186 citations · 330 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA20096 cited

On the constancy of the high-mass slope of the initial mass function

Paul C. Clark, Simon C. O. Glover, Ian A. Bonnell +1

The observed slope at the high-mass end of the initial mass function (IMF) displays a remarkable universality in a wide variety of physical environments. We predict that competitiv…

astro-ph.CO200968 cited

The influence of magnetic fields on the thermodynamics of primordial star formation

Dominik R. G. Schleicher, Daniele Galli, Simon C. O. Glover +4

We explore the effects of magnetic energy dissipation on the formation of the first stars. For this purpose, we follow the evolution of primordial chemistry in the presence of magn…

astro-ph20088 cited

Cosmic constraints rule out s-wave annihilation of light dark matter

Dominik R. G. Schleicher, Simon C. O. Glover, Robi Banerjee +1

Light dark matter annihilating into electron-positron pairs emits a significant amount of internal bremsstrahlung that may contribute to the cosmic gamma-ray background. The amount…

astro-ph200857 cited

Turbulent Mixing in the Interstellar Medium -- an application for Lagrangian Tracer Particles

C Federrath, S C O Glover, R S Klessen +1

We use 3-dimensional numerical simulations of self-gravitating compressible turbulent gas in combination with Lagrangian tracer particles to investigate the mixing process of molec…

astro-ph20075 cited

The First Stellar Cluster

Paul C. Clark, Simon C. O. Glover, Ralf S. Klessen

We report results from numerical simulations of star formation in the early universe that focus on gas at very high densities and very low metallicities. We argue that the gas in t…

astro-ph2007186 cited

Star formation at very low metallicity. I: Chemistry and cooling at low densities

S. C. O. Glover, A. -K. Jappsen

We present a simplified chemical and thermal model designed to allow computationally efficient study of the thermal evolution of metal-poor gas within large numerical simulations.…