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Showing results 5 to 16 of 16
01_Sur_The_generation_of_strong_2010.pdf.jpg

The generation of strong magnetic fields during the formation of the first stars

Author(s)Sur, Sharanya; Banerjee, Robi; Klessen, R., et al
TypeConference paper
Date Published2010
Date CreatedNovember 9-12 2010
01_Girichidis_Importance_of_the_initial_2011.pdf.jpg

Importance of the initial conditions for star formation - I. Cloud evolution and morphology

Author(s)Girichidis, Philipp; Federrath, Christoph; Banerjee, Robi, et al
TypeJournal article
Date Published2011
Date Created-
01_Federrath_Mach_number_dependence_of_2011.pdf.jpg

Mach number dependence of turbulent magnetic field amplification: Solenoidal versus compressive flows

Author(s)Federrath, Christoph; Chabrier, G.; Schober, Jennifer, et al
TypeJournal article
Date Published2011
Date Created-
01_Sur_Magnetic_field_amplification_2012.pdf.jpg

Magnetic field amplification during gravitational collapse - influence of turbulence, rotation and gravitational compression

Author(s)Sur, Sharanya; Federrath, Christoph; Schleicher, Dominik R. G., et al
TypeJournal article
Date Published2012
Date Created-
01_Micic_Modelling_H2_formation_in_the_2012.pdf.jpg

Modelling H2 formation in the turbulent interstellar medium: solenoidal versus compressive turbulent forcing

Author(s)Micic, Milica; Glover, Simon C. O.; Federrath, Christoph, et al
TypeJournal article
Date Published2012
Date Created-
01_Molina_The_density_variance-Mach_2012.pdf.jpg

The density variance-Mach number relation in supersonic turbulence - I. Isothermal, magnetized gas

Author(s)Molina, F. Z.; Glover, Simon C. O.; Federrath, Christoph, et al
TypeJournal article
Date Published2012
Date Created-
01_Peters_The_impact_of_thermodynamics_2012.pdf.jpg

The impact of thermodynamics on gravitational collapse: Filament formation and magnetic field amplification

Author(s)Peters, Thomas; Schleicher, Dominik R. G.; Klessen, R., et al
TypeJournal article
Date Published2012
Date Created-
01_Schneider_The_link_between_molecular_2011.pdf.jpg

The link between molecular cloud structure and turbulence

Author(s)Schneider, N.; Bontemps, S.; Simon, R, et al
TypeJournal article
Date Published2011
Date Created-
01_Schober_The_small-scale_dynamo_and_2012.pdf.jpg

The small-scale dynamo and non-ideal magnetohydrodynamics in primordial star formation

Author(s)Schober, Jennifer; Schleicher, Dominik R. G.; Federrath, Christoph, et al
TypeJournal article
Date Published2012
Date Created-
01_Federrath_The_star_formation_rate_of_2012.pdf.jpg

The star formation rate of turbulent magnetized clouds: Comparing theory, simulations, and observations

Author(s)Federrath, Christoph; Klessen, R.
TypeJournal article
Date Published2012
Date Created-
01_Roman-Duval_The_turbulence_spectrum_of_2011.pdf.jpg

The turbulence spectrum of molecular clouds in the galactic ring survey: A density-dependent principal component analysis calibration

Author(s)Roman-Duval, Julia; Federrath, Christoph; Brunt, C M, et al
TypeJournal article
Date Published2011
Date Created-
01_Schneider_Understanding_star_formation_2016.pdf.jpg

Understanding star formation in molecular clouds III. Probability distribution functions of molecular lines in Cygnus X

Author(s)Schneider, N; Bontemps, S.; Motte, F., et al
TypeJournal article
Date Published2016
Date Created-

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