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The small-scale dynamo: breaking universality at high Mach numbers
Dominik R G Schleicher, Jennifer Schober, Christoph Federrath, Stefano Bovino and Wolfram Schmidt New Journal of Physics 15(2) 023017 (2013) https://doi.org/10.1088/1367-2630/15/2/023017
A model for (non-lognormal) density distributions in isothermal turbulence
Magnetic fields during high redshift structure formation
D.R.G. Schleicher, M. Latif, J. Schober, W. Schmidt, S. Bovino, C. Federrath, J. Niemeyer, R. Banerjee and R.S. Klessen Astronomische Nachrichten 334(6) 531 (2013) https://doi.org/10.1002/asna.201211898
Magnetic field amplification by small-scale dynamo action: Dependence on turbulence models and Reynolds and Prandtl numbers
The linewidth-size relationship in the dense interstellar medium of the Central Molecular Zone
Rahul Shetty, Christopher N. Beaumont, Michael G. Burton, Brandon C. Kelly and Ralf S. Klessen Monthly Notices of the Royal Astronomical Society 425(1) 720 (2012) https://doi.org/10.1111/j.1365-2966.2012.21588.x
Small-scale dynamo at low magnetic Prandtl numbers
Importance of the initial conditions for star formation - III. Statistical properties of embedded protostellar clusters
Philipp Girichidis, Christoph Federrath, Richard Allison, Robi Banerjee and Ralf S. Klessen Monthly Notices of the Royal Astronomical Society 420(4) 3264 (2012) https://doi.org/10.1111/j.1365-2966.2011.20250.x
MOLECULAR TRACERS OF TURBULENT SHOCKS IN GIANT MOLECULAR CLOUDS
Jennifer Schober, Dominik R. G. Schleicher, Ralf S. Klessen, et al. Proceedings of the International Astronomical Union 8(S294) 237 (2012) https://doi.org/10.1017/S1743921313002585
The properties of the interstellar medium in disc galaxies with stellar feedback
A NEW JEANS RESOLUTION CRITERION FOR (M)HD SIMULATIONS OF SELF-GRAVITATING GAS: APPLICATION TO MAGNETIC FIELD AMPLIFICATION BY GRAVITY-DRIVEN TURBULENCE
Christoph Federrath, Sharanya Sur, Dominik R. G. Schleicher, Robi Banerjee and Ralf S. Klessen The Astrophysical Journal 731(1) 62 (2011) https://doi.org/10.1088/0004-637X/731/1/62
ANISOTROPY LENGTHENS THE DECAY TIME OF TURBULENCE IN MOLECULAR CLOUDS
THE GLOBAL EVOLUTION OF GIANT MOLECULAR CLOUDS. II. THE ROLE OF ACCRETION
Nathan J. Goldbaum, Mark R. Krumholz, Christopher D. Matzner and Christopher F. McKee The Astrophysical Journal 738(1) 101 (2011) https://doi.org/10.1088/0004-637X/738/1/101
The link between molecular cloud structure and turbulence
MOLECULAR CLOUD EVOLUTION. III. ACCRETION VERSUS STELLAR FEEDBACK
Enrique Vázquez-Semadeni, Pedro Colín, Gilberto C. Gómez, Javier Ballesteros-Paredes and Alan W. Watson The Astrophysical Journal 715(2) 1302 (2010) https://doi.org/10.1088/0004-637X/715/2/1302
THE TEMPERATURE OF INTERSTELLAR CLOUDS FROM TURBULENT HEATING
HIGH- AND LOW-MASS STAR-FORMING REGIONS FROM HIERARCHICAL GRAVITATIONAL FRAGMENTATION. HIGH LOCAL STAR FORMATION RATES WITH LOW GLOBAL EFFICIENCIES
Enrique Vázquez-Semadeni, Gilberto C. Gómez, A.-Katharina Jappsen, Javier Ballesteros-Paredes and Ralf S. Klessen The Astrophysical Journal 707(2) 1023 (2009) https://doi.org/10.1088/0004-637X/707/2/1023
THE CLUSTERING BEHAVIOR OF PRE-MAIN-SEQUENCE STARS IN NGC 346 IN THE SMALL MAGELLANIC CLOUD
The nature of the velocity field in molecular clouds - I. The non-magnetic case
Enrique Vázquez-Semadeni, Ricardo F. González, Javier Ballesteros-Paredes, Adriana Gazol and Jongsoo Kim Monthly Notices of the Royal Astronomical Society (2008) https://doi.org/10.1111/j.1365-2966.2008.13778.x
On the structure of the turbulent interstellar atomic hydrogen
The Virial Balance of Clumps and Cores in Molecular Clouds
Sami Dib, Jongsoo Kim, Enrique Vazquez‐Semadeni, Andreas Burkert and Mohsen Shadmehri The Astrophysical Journal 661(1) 262 (2007) https://doi.org/10.1086/513708
The formation of star clusters - II. 3D simulations of magnetohydrodynamic turbulence in molecular clouds
Observational Constraints on the Ages of Molecular Clouds and the Star Formation Timescale: Ambipolar‐Diffusion–controlled or Turbulence‐induced Star Formation?
Telemachos Ch. Mouschovias, Konstantinos Tassis and Matthew W. Kunz The Astrophysical Journal 646(2) 1043 (2006) https://doi.org/10.1086/500125
Hydrodynamical simulations of the decay of high-speed molecular turbulence - II. Divergence from isothermality
The Lifetimes and Evolution of Molecular Cloud Cores
Enrique Vazquez‐Semadeni, Jongsoo Kim, Mohsen Shadmehri and Javier Ballesteros‐Paredes The Astrophysical Journal 618(1) 344 (2005) https://doi.org/10.1086/425951
Adaptive Mesh Refinement - Theory and Applications
Richard I. Klein, Robert T. Fisher, Christopher F. McKee and Mark Krumholz Lecture Notes in Computational Science and Engineering, Adaptive Mesh Refinement - Theory and Applications 41 431 (2005) https://doi.org/10.1007/3-540-27039-6_32
Quiescent and Coherent Cores from Gravoturbulent Fragmentation
Ralf S. Klessen, Javier Ballesteros‐Paredes, Enrique Vazquez‐Semadeni and Carolina Duran‐Rojas The Astrophysical Journal 620(2) 786 (2005) https://doi.org/10.1086/427255
A Solution to the Pre-Main-Sequence Accretion Problem
Paolo Padoan, Alexei Kritsuk, Michael L. Norman and Åke Nordlund The Astrophysical Journal 622(1) L61 (2005) https://doi.org/10.1086/429562
Number ratios of young stellar objects in embedded clusters