Christoph Federrath
Christoph Federrath
Australian National University, Research School of Astronomy and Astrophysics
Verified email at anu.edu.au - Homepage
TitleCited byYear
The star formation rate of turbulent magnetized clouds: comparing theory, simulations, and observations
C Federrath, RS Klessen
The Astrophysical Journal 761 (2), 156, 2012
4072012
The density probability distribution in compressible isothermal turbulence: solenoidal versus compressive forcing
C Federrath, RS Klessen, W Schmidt
The Astrophysical Journal Letters 688 (2), L79, 2008
3872008
Modeling collapse and accretion in turbulent gas clouds: implementation and comparison of sink particles in AMR and SPH
C Federrath, R Banerjee, PC Clark, RS Klessen
The Astrophysical Journal 713 (1), 269, 2010
3362010
Modelling CO formation in the turbulent interstellar medium
SCO Glover, C Federrath, MM Mac Low, RS Klessen
Monthly Notices of the Royal Astronomical Society 404 (1), 2-29, 2010
2792010
A new jeans resolution criterion for (M) HD simulations of self-gravitating gas: application to magnetic field amplification by gravity-driven turbulence
C Federrath, S Sur, DRG Schleicher, R Banerjee, RS Klessen
The Astrophysical Journal 731 (1), 62, 2011
2362011
On the star formation efficiency of turbulent magnetized clouds
C Federrath, RS Klessen
The Astrophysical Journal 763 (1), 51, 2013
2322013
A comparison between grid and particle methods on the statistics of driven, supersonic, isothermal turbulence
DJ Price, C Federrath
Monthly Notices of the Royal Astronomical Society 406 (3), 1659-1674, 2010
2072010
On the universality of supersonic turbulence
C Federrath
Monthly Notices of the Royal Astronomical Society 436 (2), 1245-1257, 2013
1772013
The fractal density structure in supersonic isothermal turbulence: solenoidal versus compressive energy injection
C Federrath, RS Klessen, W Schmidt
The Astrophysical Journal 692 (1), 364, 2009
1672009
Mach number dependence of turbulent magnetic field amplification: solenoidal versus compressive flows
C Federrath, G Chabrier, J Schober, R Banerjee, RS Klessen, ...
Physical Review Letters 107 (11), 114504, 2011
1662011
Importance of the initial conditions for star formation–I. Cloud evolution and morphology
P Girichidis, C Federrath, R Banerjee, RS Klessen
Monthly Notices of the Royal Astronomical Society 413 (4), 2741-2759, 2011
1532011
What determines the density structure of molecular clouds? A case study of Orion B with Herschel
N Schneider, P André, V Könyves, S Bontemps, F Motte, C Federrath, ...
The Astrophysical Journal Letters 766 (2), L17, 2013
1522013
The density variance–Mach number relation in supersonic turbulence–I. Isothermal, magnetized gas
FZ Molina, SCO Glover, C Federrath, RS Klessen
Monthly Notices of the Royal Astronomical Society 423 (3), 2680-2689, 2012
1522012
The generation of strong magnetic fields during the formation of the first stars
S Sur, DRG Schleicher, R Banerjee, C Federrath, RS Klessen
The Astrophysical Journal Letters 721 (2), L134, 2010
1372010
Inefficient star formation through turbulence, magnetic fields and feedback
C Federrath
Monthly Notices of the Royal Astronomical Society 450 (4), 4035-4042, 2015
1202015
The density variance–mach number relation in supersonic, isothermal turbulence
DJ Price, C Federrath, CM Brunt
The Astrophysical Journal Letters 727 (1), L21, 2010
1152010
Comparing the statistics of interstellar turbulence in simulations and observations-Solenoidal versus compressive turbulence forcing
C Federrath, J Roman-Duval, RS Klessen, W Schmidt, MM Mac Low
Astronomy & Astrophysics 512, A81, 2010
1122010
Modeling jet and outflow feedback during star cluster formation
C Federrath, M Schrön, R Banerjee, RS Klessen
The Astrophysical Journal 790 (2), 128, 2014
1092014
Is the scaling of supersonic turbulence universal?
W Schmidt, C Federrath, R Klessen
Physical Review Letters 101 (19), 194505, 2008
1002008
On the universality of interstellar filaments: theory meets simulations and observations
C Federrath
Monthly Notices of the Royal Astronomical Society 457 (1), 375-388, 2016
992016
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