Vadim Semenov

Center for Astrophysics | Harvard & Smithsonian

Visualizations

Some simulations and visualizations produced during my work. Each video can be downloaded in full quality from its own controls menu, and the corresponding papers are linked from the captions.

Driven supersonic turbulence: gas density and velocity magnitudeRead more
Cosmological simulation of a Milky Way analog: gas density and small-scale turbulenceHow Early Could the Milky Way’s Disk Form?·From UV-bright Galaxies to Early Disks·Read more
Cosmological simulation of a Milky Way-like galaxy with ART and TNGHow Early Could the Milky Way’s Disk Form?·From UV-bright Galaxies to Early Disks·Read more
Disk formation in a cosmological simulation of a MW analogHow Early Could the Milky Way’s Disk Form?·From UV-bright Galaxies to Early Disks·Read more
Simulation of a galaxy with a subgrid turbulence model: young stars, gas density, temperature, and turbulent velocities on unresolved scalesThe Physical Origin of Long Gas Depletion Times·How Galaxies Form Stars·Read more
Cycling of interstellar gas between star-forming and non-star-forming statesThe Physical Origin of Long Gas Depletion Times·How Galaxies Form Stars·Read more
NGC300-like galaxy simulation with subgrid turbulence and radiative transferSpatial Decorrelation of Young Stars and Dense Gas·Read more
NGC300-like galaxy simulation — article versionSpatial Decorrelation of Young Stars and Dense Gas·Read more
Cosmic ray feedback in a gas-rich galaxy — no CRsCR Diffusion Suppression Inhibits Clump Formation·Read more
Cosmic ray feedback — CRs with constant diffusivityCR Diffusion Suppression Inhibits Clump Formation·Read more
Cosmic ray feedback — CRs with diffusivity suppressionCR Diffusion Suppression Inhibits Clump Formation·Read more