Published July 15, 2016
| Version v1
Poster
Open
The Phantom SPH code
Authors/Creators
- 1. Monash Centre for Astrophysics
- 2. University of Leicester
Description
I will present the capabilities of the Phantom SPH code for global simulations of dust and gas in protoplanetary discs. I will present our new algorithms for simulating both small and large grains in discs, as well as our progress towards simulating evolving grain populations and coupling with radiation. Finally, I will discuss our recent applications to HL Tau and the physics of dust gap opening.
Files
planets2016-PriceD_poster.pdf
Files
(6.0 MB)
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