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...
The Dynamics Of Stellar Winds: Their Structures And [oiii] Line Formation (2007)
Seung-hoon Cha, Young-jin Lee, Seung-urn Choe
To understand the dynamical structures of stellar wind bubble, one and two-dimensional calculations has been performed. Using FCT Code with cooling effects and assuming constant mass loss rate and...
An implicit method for radiative transfer with the diffusion approximation in SPH (2006)
Viau, Serge, Bastien, Pierre, Cha, Seung-Hoon
An implicit method for radiative transfer in SPH is described. The diffusion approximation is used, and the hydrodynamic calculations are performed by a fully three--dimensional SPH code. Instead of...