A Novel Approach to Visualizing Dark Matter Simulations.The formation of Population III binaries from cosmological initial conditions.The birth of a galaxy – III. Propelling reionization with the faintest galaxiesHow Small Were the First Cosmological Objects?SPECS: the kilometer-baseline far-IR interferometer in NASA's space science roadmapEvolution and Explosion of Very Massive Primordial StarsCosmological Hydrogen Reionization with Three‐dimensional Radiative TransferThe first generation of stars in the cold dark matter cosmologyCosmic reionization by stellar sources: population III starsCosmic reionization by stellar sources: Population II starsThe AGORA high-resolution galaxy simulations comparison projectReionization histories of Milky Way mass halosThe impact of inhomogeneous reionization on the satellite galaxy population of the Milky WayConnecting reionization to the local universeTwo Distinct Ancient Components in the Sculptor Dwarf Spheroidal Galaxy: First Results from the Dwarf Abundances and Radial Velocities TeamThe AGORA High-resolution Galaxy Simulations Comparison Project. II. Isolated disk testNumerical Simulations of High‐Redshift Star Formation in Dwarf GalaxiesENZO: an adaptive mesh refinement code for astrophysicsTracing the cosmic webThe properties of cosmic velocity fieldsTRACING, ANALYZING AND VISUALIZING DARK MATTER IN PHASE SPACEThe warm dark matter halo mass function below the cut-off scaleA new approach to simulating collisionless dark matter fluidsHow closely do baryons follow dark matter on large scales?Tracing the dark matter sheet in phase spaceMulti-scale initial conditions for cosmological simulationsMagnetic fields and angular momentum in population III star formationTurbulence and small scale dynamo action in population III star formationMagnetic fields in population III star formationThe HiiRegion of a Primordial StarThe H II Region of a Primordial StarAchieving Extreme Resolution in Numerical Cosmology Using Adaptive Mesh Refinement: Resolving Primordial Star FormationSimulations of Pregalactic Structure Formation with Radiative FeedbackAchieving extreme resolution in numerical cosmology using adaptive mesh refinementThe Formation and Fragmentation of Primordial Molecular CloudsFirst Structure Formation and the First StarsFrom cosmological initial conditions to primordial protostellar cloud coresIntroducing Enzo, an AMR Cosmology ApplicationComparing numerical methods for isothermal magnetized supersonic turbulenceDynamical Expansion of HII Regions From Ultracompact to Compact Sizes in Turbulent, Self-Gravitating Molecular Clouds
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description
Ameerika Ühendriikide astronoom
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American astronomer
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Duits astronoom
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astronom american
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astronom amerikan
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Tom Abel
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Tom Abel
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Tom Abel
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Thomas Georg Abel
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Tom Abel
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Tom Abel
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Tom Abel
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Tom Abel
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Tom Abel
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