Radiation-hydrodynamical simulations of massive star formation using Monte Carlo radiative transfer II. The formation of a 25 solar-mass star (2017)
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.1706.04017
Publication URI: https://arxiv.org/abs/1706.04017
Type: Other