Dynamic Monte Carlo radiation transfer in SPH. Radiation pressure force implementation (2009)
Nayakshin, Sergei, Cha, Seung-Hoon, Hobbs, Alexander
We present a new framework for radiation hydrodynamics simulations. Gas dynamics is modelled by the Smoothed Particle Hydrodynamics (SPH) method, whereas radiation transfer is simulated via a...
Hobbs, Alexander, Nayakshin, Sergei
Young massive stars in the central parsec of our Galaxy are best explained by star formation within at least one, and possibly two, massive self-gravitating gaseous discs. With help of numerical...
Nayakshin, Sergei, Hobbs, Alexander
Young massive stars in the central parsec of our Galaxy are best explained by star formation within at least one, and possibly two, massive self-gravitating gaseous discs. With help of numerical...