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20012009
most citedStar formation at very low metallicity. I: Chemistry and cooling at low densities

186 citations · 975 across the 16 of their papers we have counts for

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13 papers · 1 filter

astro-ph2008★ 103 cited

Algorithmic comparisons of decaying, isothermal, supersonic turbulence

S. Kitsionas, C. Federrath, R. Klessen +10

Contradicting results have been reported in the literature with respect to the performance of the numerical techniques employed for the study of supersonic turbulence. We aim at ch…

astro-ph2008★ 53 cited

Star Formation at Very Low Metallicity. V. The Greater Importance of Initial Conditions Compared to Metallicity Thresholds

A. -K. Jappsen, M. -M. Mac Low, S. C. O. Glover +2

The formation of the first stars out of metal-free gas appears to result in stars at least an order of magnitude more massive than in the present-day case. We here consider what co…

astro-ph2008★ 7 cited

The formation of the first galaxies and the transition to low-mass star formation

Thomas H. Greif, Dominik R. G. Schleicher, Jarrett L. Johnson +6

The formation of the first galaxies at redshifts z ~ 10-15 signaled the transition from the simple initial state of the universe to one of ever increasing complexity. We here revie…

astro-ph2008

Massive Star Forming Regions: Turbulent Support or Global Collapse?

Enrique Vazquez-Semadeni, Javier Ballesteros-Paredes, Ralf S. Klessen +1

We present preliminary numerical evidence that the physical conditions in high-mass star forming regions can arise from global gravitational infall, with the velocity dispersions b…

astro-ph2007★ 54 cited

Star Formation at Very Low Metallicity. IV. Fragmentation Does Not Depend on Metallicity for Cold Initial Conditions

Anne-Katharina Jappsen, Ralf S. Klessen, Simon C. O. Glover +1

Primordial star formation appears to result in stars at least an order of magnitude more massive than modern star formation. It has been proposed that the transition from primordia…

astro-ph2007★ 1 cited

The Influence of Metallicity on Star Formation in Protogalaxies

A. -K. Jappsen, S. C. O. Glover, R. S. Klessen +1

In cold dark matter cosmological models, the first stars to form are believed to do so within small protogalaxies. We wish to understand how the evolution of these early protogalax…