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astro-ph.SR2024
Introducing two improved methods for approximating radiative cooling in hydrodynamical simulations of accretion discs
Alison K. Young, Maggie Celeste, Richard A. Booth +4
The evolution of many astrophysical systems depends strongly on the balance between heating and cooling, in particular star formation in giant molecular clouds and the evolution of…
astro-ph.EP2024★ 1 cited
The Role of Drag and Gravity on Dust Concentration in a Gravitationally Unstable Disc
Sahl Rowther, Rebecca Nealon, Farzana Meru +5
We carry out three dimensional smoothed particle hydrodynamics simulations to study the role of gravitational and drag forces on the concentration of large dust grains (St > 1) in…