Collapse of a molecular cloud core to stellar densities: stellar-core and outflow formation in radiation magnetohydrodynamic simulations (2014)
Attributed to:
The formation of stars and planets: Radiation hydrodynamical and magnetohydrodynamical simulations
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stt1865
Publication URI: http://dx.doi.org/10.1093/mnras/stt1865
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1