Mark R. Krumholz
educated at: University of California, Berkeley, Princeton University
occupation: astronomer
award received: Australian Laureate Fellowship
official website: www.mso.anu.edu.au/~krumholz
Articles 119
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The Volatile Carbon-to-oxygen Ratio as a Tracer for the Formation Locations of Interstellar Comets
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ORION2: A magnetohydrodynamics code for star formation
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The dependence of the hierarchical distribution of star clusters on galactic environment
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Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
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The major mechanism to drive turbulence in star-forming galaxies
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The diffuse γ-ray background is dominated by star-forming galaxies
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Testing the turbulent origin of the stellar initial mass function
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Reconstructing three-dimensional densities from two-dimensional observations of molecular gas
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The physics of gas phase metallicity gradients in galaxies
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On the origin of nitrogen at low metallicity
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Evolution of Stellar Feedback in H ii Regions
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Cosmic rays across the star-forming galaxy sequence – I. Cosmic ray pressures and calorimetry
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Cosmic rays across the star-forming galaxy sequence – II. Stability limits and the onset of cosmic ray-driven outflows
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Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMF
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The life cycle of the Central Molecular Zone - II. Distribution of atomic and molecular gas tracers
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Distribution and kinematics of 26Al in the Galactic disc
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The Catalogue for Astrophysical Turbulence Simulations (CATS)
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An uncertainty principle for star formation – III. The characteristic emission time-scales of star formation rate tracers
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An uncertainty principle for star formation – V. The influence of dust extinction on star formation rate tracer lifetimes and the inferred molecular cloud lifecycle
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Which feedback mechanisms dominate in the high-pressure environment of the central molecular zone?
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Dynamics of small grains in transitional discs
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Understanding biases in measurements of molecular cloud kinematics using line emission
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The importance of magnetic fields for the initial mass function of the first stars
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Formation and evolution of the local interstellar environment: combined constraints from nucleosynthetic and X-ray data
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The Role of Outflows, Radiation Pressure, and Magnetic Fields in Massive Star Formation
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Quantifying the effects of spatial resolution and noise on galaxy metallicity gradients
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The SAMI galaxy survey: gas velocity dispersions in low-z star-forming galaxies and the drivers of turbulence
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Helium and nitrogen enrichment in massive main-sequence stars: mechanisms and implications for the origin of WNL stars
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How do bound star clusters form?
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Cosmic ray transport in starburst galaxies
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A fundamental test for stellar feedback recipes in galaxy simulations
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Star Clusters Across Cosmic Time
Human - wd:Q42698575