Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H ii regions - spherically symmetric ionized accretion flows (2019)
Attributed to:
Astronomy at St Andrews 2018-2021
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stz621
Publication URI: http://dx.doi.org/10.1093/mnras/stz621
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 3