
development of density and size scales during the collapse. No dust model (opacities, size distribution etc.) is assumed for the ray tracer. The colours seen in the image do not correspond to any actual wavelengths. The density calculated by the SPH code is translated into a scattering and absorbing medium. Rayleigh scattering is modelled with scattering coefficients of 0.5 for the "red" channel, 0.7 for the "green" channel, and 0.9 for the "blue" channel. The same coefficients are applied ...
Author: Astropov; Tags:
Astronomy
Astrophysics
Star Formation
Numerical Simulation
raytracing
M16