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The role of three-body H2 formation in the fragmentation of primordial gas
Oxford University Press | 2015| -
On the effects of rotation during the formation of population III protostars
American Institute of Physics | 2012| -
Star Formation in Isolated Disk Galaxies. I. Models and Characteristics of Nonlinear Gravitational Collapse
Free accessArXiv | 2005| -
The formation of direct collapse black holes under the influence of streaming velocities
Free accessArXiv | 2017| -
On the nature of star-forming filaments: II. Sub-filaments and velocities
Free accessArXiv | 2015| -
Modeling H2 formation in the turbulent ISM: Solenoidal versus compressive turbulent forcing
Free accessArXiv | 2011| -
On the nature of star-forming filaments - II. Subfilaments and velocities
Oxford University Press | 2015| -
The relation between the turbulent Mach number and observed fractal dimensions of turbulent clouds
Free accessBASE | 2019| -
On the effects of rotation during the formation of population III protostars
Free accessArXiv | 2012| -
Star Formation in Isolated Disk Galaxies. II. Schmidt Laws and Efficiency of Gravitational Collapse
Free accessArXiv | 2005|
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