Comparison of two- and three-dimensional compressible convection in a pre-main sequence star (2020)
Attributed to:
A comprehensive study of stars, disks and exoplanets
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2003.04643
Publication URI: https://arxiv.org/abs/2003.04643
Type: Other