Comparison of 2D and 3D compressible convection in a pre-main sequence star (2020)
Attributed to:
DiRAC 3 Operations
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201834736
Publication URI: http://dx.doi.org/10.1051/0004-6361/201834736
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics