Three-dimensional SPH simulations of accretion discs
classification
🌌 astro-ph
keywords
discsaccretionevenpolytropicsimulationsalwaysappearbalance
read the original abstract
We discuss some 3D numerical simulations of accretion discs using the SPH method and a polytropic equation of state. We show that discs exist even for as large value of the polytropic index as 1.2, and that these discs are always in hydrostatic balance. We also show that even without any inflow, spiral shocks appear in the discs.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.