Norman, Michael L.
Michael L. Norman
VIAF ID: 3174629 (Personal)
Permalink: http://viaf.org/viaf/3174629
Preferred Forms
- 100 0 _ ‡a Michael L. Norman
- 100 1 _ ‡a Norman, Michael L. (sparse)
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- 100 1 _ ‡a Norman, Michael L.
- 100 1 _ ‡a Norman, Michael L.
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- 100 1 _ ‡a Norman, Michael L.
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4xx's: Alternate Name Forms (4)
Works
Title | Sources |
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Achieving extreme resolution in numerical cosmology using adaptive mesh refinement | |
The AGORA high-resolution galaxy simulations comparison project | |
Astrophysical radiation hydrodynamics | |
Baryons in the Warm‐Hot Intergalactic Medium | |
The Biermann Battery in Cosmological MHD Simulations of Population III Star Formation | |
The birth of a galaxy – III. Propelling reionization with the faintest galaxies | |
Comparing AMR and SPH Cosmological Simulations. I. Dark Matter and Adiabatic Simulations | |
Comparing numerical methods for isothermal magnetized supersonic turbulence | |
A Cosmological AMR MHD Module for Enzo | |
Cosmological Hydrogen Reionization with Three‐dimensional Radiative Transfer | |
Cosmological magnetohydrodynamic simulations of galaxy cluster radio relics: insights and warnings for observations | |
Cosmological Parameters σ8, the Baryon Density Ωb, the Vacuum Energy Density ΩΛ, the Hubble Constant and the UV Background Intensity from a Calibrated Measurement of HiLyα Absorption atz = 1.9 | |
Cosmological radiative transfer codes comparison project – I. The static density field tests | |
The effect of projection on derived mass-size and linewidth-size relationships | |
ENZO: an adaptive mesh refinement code for astrophysics | |
Evolution and distribution of magnetic fields from active galactic nuclei in galaxy clusters. I. The effect of injection energy and redshift | |
First Structure Formation and the First Stars | |
The Formation and Fragmentation of Primordial Molecular Clouds | |
Formation of Cool Cores in Galaxy Clusters via Hierarchical Mergers | |
From cosmological initial conditions to primordial protostellar cloud cores | |
Hydrodynamical Simulations of the Lyα Forest: Model Comparisons | |
Introducing Enzo, an AMR Cosmology Application | |
Numerical Simulations of High‐Redshift Star Formation in Dwarf Galaxies | |
A piecewise parabolic method for cosmological hydrodynamics | |
Resolving the Lyα Forest | |
The Role of the First Metals in Forming the Second Stars | |
Simulating Cosmological Evolution with Enzo | |
Simulating Radiating and Magnetized Flows in Multiple Dimensions with ZEUS‐MP | |
Spectral Analysis of the Lyα Forest in a Cold Dark Matter Cosmology | |
Statistical Properties of X‐Ray Clusters: Analytic and Numerical Comparisons | |
Structured Adaptive Mesh Refinement (SAMR) Grid Methods | |
Three Modes of Metal-Enriched Star Formation in the Early Universe | |
Turbulence and dynamo in galaxy cluster medium: implications on the origin of cluster magnetic fields | |
The two states of star-forming clouds | |
A Universal Temperature Profile for Galaxy Clusters | |
Weak Gravitational Lensing and Cluster Mass Estimates | |
WFPC2 Studies of the Crab Nebula. III. Magnetic Rayleigh-Taylor Instabilities and the Origin of the Filaments | |
X-ray clusters from a high-resolution hydrodynamic PPM simulation of the cold dark matter universe | |
The X-Ray Luminosity Function and Gas Mass Function for Optically Selected Poor and Rich Clusters of Galaxies |