Radiation-hydrodynamical simulations of massive star formation using Monte Carlo radiative transfer - II. The formation of a 25 solar-mass star (2017)
Attributed to:
Supercomputer support for the Astrophysics Group at the University of Exeter
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stx1490
Publication URI: http://dx.doi.org/10.1093/mnras/stx1490
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 4