Dust Scattering in Protoplanetary Disks

Daniel Devlin
Using the Monte Carlo radiative transfer method, the following code, written in C++ and building on the Athena++ framework, adds a program for dust scattering simulations. We then compare the output of the code to a tested dust simulation code written in FORTRAN. For this comparison we use a problem generator which simulates a protoplanetary disc of varying density which surrounds a binary star system with the stars having different luminosities. We then discuss the...
This data repository is not currently reporting usage information. For information on how your repository can submit usage information, please see our documentation.