Christoph Federrath

Identifiers

• name variant Christoph Federrath 0.60 · backfill

Papers (102)

1. Computational advances and challenges in simulations of turbulence and star formation astro-ph.GA · 2025 · author #1
2. Rest-frame UV and optical emission line diagnostics of ionised gas properties: a test case in a star-forming knot of a lensed galaxy at z~1.7 astro-ph.GA · 2019 · author #7
3. The relation between the turbulent Mach number and observed fractal dimensions of turbulent clouds astro-ph.GA · 2019 · author #2
4. Testing Star Formation Laws on Spatially Resolved Regions in a $z \approx 4.3$ Starburst Galaxy astro-ph.GA · 2019 · author #3
5. Through thick or thin: Multiple components of the magneto-ionic medium towards the nearby ${\rm H\,{\small II}}$ region Sharpless 2-27 revealed by Faraday tomography astro-ph.GA · 2019 · author #8
6. The relation between the true and observed fractal dimensions of turbulent clouds astro-ph.GA · 2019 · author #2
7. Tiny Grains Shining Bright in the Gaps of Herbig Ae Transitional Discs astro-ph.EP · 2019 · author #3
8. The role of initial magnetic field structure in the launching of protostellar jets astro-ph.SR · 2019 · author #2
9. The SAMI Galaxy Survey: Bayesian Inference for Gas Disk Kinematics using a Hierarchical Gaussian Mixture Model astro-ph.GA · 2019 · author #8
10. The metallicity and elemental abundance maps of kinematically atypical galaxies for constraining minor merger and accretion histories astro-ph.GA · 2019 · author #3
11. The Role of Magnetic Fields in Setting the Star Formation Rate and the Initial Mass Function astro-ph.GA · 2019 · author #2
12. The SAMI Galaxy Survey: Quenching of star formation in clusters I. Transition galaxies astro-ph.GA · 2019 · author #11
13. On the dynamics and survival of fractal clouds in galactic winds astro-ph.GA · 2019 · author #3
14. The impact of black hole seeding in cosmological simulations astro-ph.GA · 2018 · author #3
15. On the shape and completeness of the column density probability distribution function of molecular clouds astro-ph.GA · 2018 · author #2
16. The role of turbulence during the formation of circumbinary discs astro-ph.EP · 2018 · author #2
17. A new method for probing magnetic field strengths from striations in the interstellar medium astro-ph.GA · 2018 · author #2
18. Magnetic field tomography in two clouds towards Ursa Major using HI fibers astro-ph.GA · 2018 · author #2
19. The SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added products astro-ph.GA · 2018 · author #23
20. Multiplicity of disc-bearing stars in Upper Scorpius and Upper Centaurus-Lupus astro-ph.EP · 2018 · author #5
21. Ghost of a Shell: Magnetic Fields of Galactic Supershell GSH 006$-$15$+$7 astro-ph.GA · 2018 · author #3
22. The turbulent formation of stars astro-ph.SR · 2018 · author #1
23. The origin of kinematically distinct cores and misaligned gas discs in galaxies from cosmological simulations astro-ph.GA · 2018 · author #2
24. Isothermal Fragmentation: Is there a low-mass cut-off? astro-ph.GA · 2018 · author #5
25. Numerical Calibration of the HCN$-$Star Formation Correlation astro-ph.GA · 2018 · author #3
26. The SAMI Galaxy Survey: Spatially Resolving the Main Sequence of Star Formation astro-ph.GA · 2018 · author #25
27. Testing Star Formation Laws in a Starburst Galaxy At Redshift 3 Resolved with ALMA astro-ph.GA · 2017 · author #2
28. Relationship between turbulence energy and density variance in the Solar neighbourhood molecular clouds astro-ph.GA · 2017 · author #2
29. The most ancient spiral galaxy: a 2.6-Gyr-old disk with a tranquil velocity field astro-ph.GA · 2017 · author #4
30. The effect of photoionising feedback on star formation in isolated and colliding clouds astro-ph.GA · 2017 · author #3
31. The SAMI Galaxy Survey: Global stellar populations on the size-mass plane astro-ph.GA · 2017 · author #11
32. Filament formation in wind-cloud interactions. II. Clouds with turbulent density, velocity, and magnetic fields astro-ph.GA · 2017 · author #2
33. The SAMI Galaxy Survey: energy sources of the turbulent velocity dispersion in spatially-resolved local star-forming galaxies astro-ph.GA · 2017 · author #2
34. Compression of turbulent magnetized gas in Giant Molecular Clouds astro-ph.GA · 2017 · author #2
35. Binary Star Formation and the Outflows from their Discs astro-ph.SR · 2017 · author #2
36. Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times10^{10}$ M$_\odot$ astro-ph.GA · 2017 · author #2
37. Adaptive mesh refinement simulations of a galaxy cluster merger - I. Resolving and modelling the turbulent flow in the cluster outskirts astro-ph.CO · 2017 · author #2
38. On the effective turbulence driving mode of molecular clouds formed in disc galaxies astro-ph.GA · 2017 · author #3
39. The SAMI Galaxy Survey: a new method to estimate molecular gas surface densities from star formation rates astro-ph.GA · 2017 · author #1
40. The driving of turbulence in simulations of molecular cloud formation and evolution astro-ph.GA · 2017 · author #2
41. Parallel Implementation of Lossy Data Compression for Temporal Data Sets cs.DC · 2017 · author #4
42. Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics astro-ph.IM · 2017 · author #19
43. Magnetic field amplification in turbulent astrophysical plasmas physics.plasm-ph · 2016 · author #1
44. Extreme Scale-out SuperMUC Phase 2 - lessons learned cs.DC · 2016 · author #26
45. SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds astro-ph.GA · 2016 · author #2
46. The world's largest turbulence simulations astro-ph.SR · 2016 · author #1
47. The role of turbulence, magnetic fields and feedback for star formation astro-ph.GA · 2016 · author #1
48. The small-scale turbulent dynamo in smoothed particle magnetohydrodynamics astro-ph.IM · 2016 · author #3
49. A comparison between grid and particle methods on the small-scale dynamo in magnetised supersonic turbulence astro-ph.IM · 2016 · author #3
50. The reliability of observational measurements of column density probability distribution functions astro-ph.IM · 2016 · author #4
51. On the universality of interstellar filaments: theory meets simulations and observations astro-ph.SR · 2015 · author #1
52. Filament formation in wind-cloud interactions. I. Spherical clouds in uniform magnetic fields astro-ph.GA · 2015 · author #3
53. Saturation of the Turbulent Dynamo physics.plasm-ph · 2015 · author #3
54. A universal, turbulence-regulated star formation law: from Milky Way clouds to high-redshift disk and starburst galaxies astro-ph.GA · 2015 · author #2
55. The density variance - Mach number relation in isothermal and non-isothermal adiabatic turbulence astro-ph.GA · 2015 · author #2
56. Inefficient star formation through turbulence, magnetic fields and feedback astro-ph.SR · 2015 · author #1
57. Nonlinear closures for scale separation in supersonic magnetohydrodynamic turbulence physics.flu-dyn · 2015 · author #5
58. The density structure and star formation rate of non-isothermal polytropic turbulence astro-ph.GA · 2014 · author #1
59. The Turbulent Dynamo in Highly Compressible Supersonic Plasmas astro-ph.GA · 2014 · author #1
60. Modeling jet and outflow feedback during star cluster formation astro-ph.SR · 2014 · author #1
61. Collective outflow from a small multiple stellar system astro-ph.SR · 2014 · author #5
62. Principal Component Analysis of Molecular Clouds: Can CO reveal the dynamics? astro-ph.SR · 2014 · author #6
63. The Star Formation Rate of Molecular Clouds astro-ph.GA · 2013 · author #2
64. Smoothed Particle Magnetohydrodynamics Simulations of Protostellar Jets and Turbulent Dynamos astro-ph.SR · 2013 · author #3
65. A measurement of the turbulence-driven density distribution in a non-star-forming molecular cloud astro-ph.GA · 2013 · author #2
66. The origin of physical variations in the star formation law astro-ph.GA · 2013 · author #1
67. On the universality of supersonic turbulence astro-ph.SR · 2013 · author #1
68. Connection between dense gas mass fraction, turbulence driving, and star formation efficiency of molecular clouds astro-ph.GA · 2013 · author #2
69. The small-scale dynamo: Breaking universality at high Mach numbers astro-ph.CO · 2013 · author #3
70. On the Star Formation Efficiency of Turbulent Magnetized Clouds astro-ph.SR · 2012 · author #1
71. Magnetic fields during high redshift structure formation astro-ph.CO · 2012 · author #6
72. Small-Scale Dynamo Action in Primordial Halos astro-ph.CO · 2012 · author #4
73. The impact of thermodynamics on gravitational collapse: filament formation and magnetic field amplification astro-ph.GA · 2012 · author #5
74. The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and Observations astro-ph.SR · 2012 · author #1
75. A new density variance - Mach number relation for subsonic and supersonic, isothermal turbulence astro-ph.SR · 2012 · author #3
76. Star Formation in the First Galaxies I: Collapse Delayed by Lyman-Werner Radiation astro-ph.CO · 2012 · author #3
77. The Small-Scale Dynamo and Non-Ideal MHD in Primordial Star Formation astro-ph.CO · 2012 · author #3
78. Generation of strong magnetic fields via the small-scale dynamo during the formation of the first stars astro-ph.CO · 2012 · author #3
79. Magnetic field amplification during gravitational collapse - Influence of initial conditions on dynamo evolution and saturation astro-ph.SR · 2012 · author #2
80. Statistical analysis of the mass-to-flux ratio in turbulent cores: effects of magnetic field reversals and dynamo amplification astro-ph.SR · 2011 · author #2
81. Importance of the Initial Conditions for Star Formation - III: Statistical Properties of Embedded Protostellar Clusters astro-ph.SR · 2011 · author #2
82. Statistical properties of supersonic turbulence in the Lagrangian and Eulerian frameworks physics.flu-dyn · 2011 · author #2
83. MHD simulations of a supernova-driven ISM and the warm ionized medium using a positivity preserving ideal MHD scheme astro-ph.GA · 2011 · author #8
84. Magnetic fields in the first galaxies: Dynamo amplification and limits from reionization astro-ph.CO · 2011 · author #3
85. Importance of the Initial Conditions for Star Formation - II. Fragmentation Induced Starvation and Accretion Shielding astro-ph.SR · 2011 · author #2
86. Magnetic Field Amplification by Small-Scale Dynamo Action: Dependence on Turbulence Models and Reynolds and Prandtl Numbers astro-ph.CO · 2011 · author #3
87. The Turbulence Spectrum of Molecular Clouds in the Galactic Ring Survey: A Density-Dependent PCA Calibration astro-ph.GA · 2011 · author #2
88. Comparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence astro-ph.SR · 2011 · author #8
89. Modeling H2 formation in the turbulent ISM: Solenoidal versus compressive turbulent forcing astro-ph.SR · 2011 · author #3
90. Magnetic fields during primordial star formation astro-ph.CO · 2011 · author #5
91. A new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulence astro-ph.SR · 2011 · author #1
92. A robust numerical scheme for highly compressible magnetohydrodynamics: Nonlinear stability, implementation and tests astro-ph.IM · 2011 · author #2
93. Importance of the Initial Conditions for Star Formation - I. Cloud Evolution and Morphology astro-ph.SR · 2010 · author #2
94. The generation of strong magnetic fields during the formation of the first stars astro-ph.CO · 2010 · author #4
95. Implementing and comparing sink particles in AMR and SPH astro-ph.IM · 2010 · author #1
96. A method for reconstructing the PDF of a 3D turbulent density field from 2D observations astro-ph.GA · 2010 · author #2
97. Numerical and semi-analytic core mass distributions in supersonic isothermal turbulence astro-ph.SR · 2010 · author #3
98. Modeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPH astro-ph.SR · 2010 · author #1
99. Is the Scaling of Supersonic Turbulence Universal? astro-ph · 2008 · author #2
100. Numerical simulations of compressively driven interstellar turbulence: I. Isothermal gas astro-ph · 2008 · author #2
101. The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal versus Compressive Forcing astro-ph · 2008 · author #1
102. The Fractal Density Structure in Supersonic Isothermal Turbulence: Solenoidal versus Compressive Energy Injection astro-ph · 2007 · author #1

Mentions

• 1506.02182 #3 · backfill · confidence 0.70 Christoph Federrath
• 1505.03144 #2 · backfill · confidence 0.70 Christoph Federrath
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• 1406.3625 #1 · backfill · confidence 0.70 Christoph Federrath
• 1404.5463 #5 · backfill · confidence 0.70 Christoph Federrath
• 1402.2101 #6 · backfill · confidence 0.70 Christoph Federrath
• 1312.5365 #2 · backfill · confidence 0.70 Christoph Federrath
• 1310.4567 #3 · backfill · confidence 0.70 Christoph Federrath
• 1310.0809 #2 · backfill · confidence 0.70 Christoph Federrath
• 1307.1467 #1 · backfill · confidence 0.70 Christoph Federrath
• 1306.3989 #1 · backfill · confidence 0.70 Christoph Federrath
• 1304.5036 #2 · backfill · confidence 0.70 Christoph Federrath
• 1301.4371 #3 · backfill · confidence 0.70 Christoph Federrath
• 1211.6433 #1 · backfill · confidence 0.70 Christoph Federrath
• 1211.4356 #6 · backfill · confidence 0.70 Christoph Federrath
• 1210.7751 #4 · backfill · confidence 0.70 Christoph Federrath
• 1209.5861 #5 · backfill · confidence 0.70 Christoph Federrath
• 1209.2856 #1 · backfill · confidence 0.70 Christoph Federrath
• 1206.4524 #3 · backfill · confidence 0.70 Christoph Federrath
• 1205.3835 #3 · backfill · confidence 0.70 Christoph Federrath
• 1204.0658 #3 · backfill · confidence 0.70 Christoph Federrath
• 1202.4536 #3 · backfill · confidence 0.70 Christoph Federrath
• 1202.3206 #2 · backfill · confidence 0.70 Christoph Federrath
• 1111.5539 #2 · backfill · confidence 0.70 Christoph Federrath
• 1111.5440 #2 · backfill · confidence 0.70 Christoph Federrath
• 1111.2748 #2 · backfill · confidence 0.70 Christoph Federrath
• 1110.6527 #8 · backfill · confidence 0.70 Christoph Federrath
• 1110.2880 #3 · backfill · confidence 0.70 Christoph Federrath
• 1110.1924 #2 · backfill · confidence 0.70 Christoph Federrath
• 1109.4571 #3 · backfill · confidence 0.70 Christoph Federrath
• 1107.4569 #2 · backfill · confidence 0.70 Christoph Federrath
• 1103.5525 #8 · backfill · confidence 0.70 Christoph Federrath
• 1103.3056 #3 · backfill · confidence 0.70 Christoph Federrath
• 1102.3558 #5 · backfill · confidence 0.70 Christoph Federrath
• 1102.0266 #1 · backfill · confidence 0.70 Christoph Federrath
• 1101.3007 #2 · backfill · confidence 0.70 Christoph Federrath
• 1008.5255 #2 · backfill · confidence 0.70 Christoph Federrath
• 1008.3481 #4 · backfill · confidence 0.70 Christoph Federrath
• 1007.2504 #1 · backfill · confidence 0.70 Christoph Federrath
• 1003.4151 #2 · backfill · confidence 0.70 Christoph Federrath
• 1002.2359 #3 · backfill · confidence 0.70 Christoph Federrath
• 1001.4456 #1 · backfill · confidence 0.70 Christoph Federrath
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• 0808.0605 #1 · backfill · confidence 0.70 Christoph Federrath
• 0710.1359 #1 · backfill · confidence 0.70 Christoph Federrath

Frequent Coauthors

• Ralf S. Klessen 31 shared papers
• Robi Banerjee 21 shared papers
• Dominik R. G. Schleicher 9 shared papers
• Wolfram Schmidt 9 shared papers
• Jennifer Schober 8 shared papers
• Anne M. Medling 7 shared papers
• Joss Bland-Hawthorn 6 shared papers
• Julia J. Bryant 6 shared papers
• Matt S. Owers 6 shared papers
• Michael Goodwin 6 shared papers
• Nicholas Scott 6 shared papers
• Ralf Klessen 6 shared papers
• Samuel N. Richards 6 shared papers
• Scott M. Croom 6 shared papers
• Sharanya Sur 6 shared papers
• Brent Groves 5 shared papers
• Daniel J. Price 5 shared papers
• Jesse van de Sande 5 shared papers
• Lisa J. Kewley 5 shared papers
• Stefano Bovino 5 shared papers