Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars (2022)

First Author: Rizzuti F

Attributed to: DiRAC 2.5 Operations 2017-2020 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stac1981

Publication URI: http://dx.doi.org/10.1093/mnras/stac1981

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3