Publication data of Federrath, Christoph: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion200820102012201420162018202020222024050010001500200025003000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications200820102012201420162018202020222024020406080100048121620
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion200820102012201420162018202020222024051015202530
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe density variance -- Mach number relation in supersonic, isothermal turbulenceThe density variance -- Mach number relation in supersonic, isothermal turbu…On the Star Formation Efficiency of Turbulent Magnetized CloudsThe Turbulent Dynamo in Highly Compressible Supersonic PlasmasComparing Numerical Methods for Isothermal Magnetized Supersonic TurbulenceComparing Numerical Methods for Isothermal Magnetized Supersonic Turbule…Algorithmic comparisons of decaying, isothermal, compressible turbulence. I. Low-resolution simulations with fixed gridsAlgorithmic comparisons of decaying, isothermal, compressible turbulence. I.…Star Formation in the First Galaxies I: Collapse Delayed by Lyman-Werner RadiationStar Formation in the First Galaxies I: Collapse Delayed by Lyman-Werner Rad…On the universality of supersonic turbulenceFractal Density Distribution of Interstellar Clouds from Numerical Simulations of Compressively Driven Supersonic TurbulenceFractal Density Distribution of Interstellar Clouds from Numerical Simulations …The Small-Scale Dynamo and Non-Ideal MHD in Primordial Star FormationMach Number Dependence of Turbulent Magnetic Field Amplification: Solenoidal versus Compressive FlowsMach Number Dependence of Turbulent Magnetic Field Amplification: Solenoi…Numerical simulations of compressively driven interstellar turbulence: I. Isothermal gasNumerical simulations of compressively driven interstellar turbulence: I. Isoth…Modelling CO formation in the turbulent interstellar mediumA comparison between grid and particle methods on the statistics of driven, supersonic, isothermal turbulenceA comparison between grid and particle methods on the statistics of driven, …The generation of strong magnetic fields during the formation of the first starsThe generation of strong magnetic fields during the formation of the first sta…Modeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPHModeling Collapse and Accretion in Turbulent Gas Clouds: Implementation an…The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and ObservationsThe Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, …A new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulenceA new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: …The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal vs Compressive ForcingThe Density Probability Distribution in Compressible Isothermal Turbulence: S…Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcingComparing the statistics of interstellar turbulence in simulations and observa…200820102012201420162018202020222024050010001500200025003000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The density variance -- Mach number relation in supersonic, isothermal turbulenceThe density variance -- Mach number relation in supersonic, isothermal turbu…On the Star Formation Efficiency of Turbulent Magnetized CloudsThe Turbulent Dynamo in Highly Compressible Supersonic PlasmasComparing Numerical Methods for Isothermal Magnetized Supersonic TurbulenceComparing Numerical Methods for Isothermal Magnetized Supersonic Turbule…Algorithmic comparisons of decaying, isothermal, compressible turbulence. I. Low-resolution simulations with fixed gridsAlgorithmic comparisons of decaying, isothermal, compressible turbulence. I.…Star Formation in the First Galaxies I: Collapse Delayed by Lyman-Werner RadiationStar Formation in the First Galaxies I: Collapse Delayed by Lyman-Werner Rad…On the universality of supersonic turbulenceFractal Density Distribution of Interstellar Clouds from Numerical Simulations of Compressively Driven Supersonic TurbulenceFractal Density Distribution of Interstellar Clouds from Numerical Simulations …The Small-Scale Dynamo and Non-Ideal MHD in Primordial Star FormationMach Number Dependence of Turbulent Magnetic Field Amplification: Solenoidal versus Compressive FlowsMach Number Dependence of Turbulent Magnetic Field Amplification: Solenoi…Numerical simulations of compressively driven interstellar turbulence: I. Isothermal gasNumerical simulations of compressively driven interstellar turbulence: I. Isoth…Modelling CO formation in the turbulent interstellar mediumA comparison between grid and particle methods on the statistics of driven, supersonic, isothermal turbulenceA comparison between grid and particle methods on the statistics of driven, …The generation of strong magnetic fields during the formation of the first starsThe generation of strong magnetic fields during the formation of the first sta…Modeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPHModeling Collapse and Accretion in Turbulent Gas Clouds: Implementation an…The Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, Simulations, and ObservationsThe Star Formation Rate of Turbulent Magnetized Clouds: Comparing Theory, …A new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulenceA new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: …The Density Probability Distribution in Compressible Isothermal Turbulence: Solenoidal vs Compressive ForcingThe Density Probability Distribution in Compressible Isothermal Turbulence: S…Comparing the statistics of interstellar turbulence in simulations and observations: Solenoidal versus compressive turbulence forcingComparing the statistics of interstellar turbulence in simulations and observa…2008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2008201020122014201620182020202220240100200300400500