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Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H ii regions - spherically symmetric ionized accretion flows (2019)

First Author: Lund K

Attributed to: Astronomy at St Andrews 2015-2018 funded by STFC

Abstract

No abstract provided

Bibliographic Information

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