Modelling massive-star feedback with Monte Carlo radiation hydrodynamics: photoionization and radiation pressure in a turbulent cloud (2018)

First Author: Ali A

Attributed to: The formation, structure, and evolution of molecular clouds, stars, and planets funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1804.07309

Publication URI: https://arxiv.org/abs/1804.07309

Type: Other