Radiation hydrodynamic simulations of massive star formation via gravitationally trapped HII regions - Spherically symmetric ionised accretion flows (2019)
Attributed to:
Astronomy at St Andrews 2015-2018
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1903.00486
Publication URI: https://arxiv.org/abs/1903.00486
Type: Other