MHD modelling of a disc wind from a high-mass protobinary: the case of Orion Source I (2013)
Attributed to:
Star Formation and Protoplanetary Discs
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnrasl/sls021
Publication URI: http://dx.doi.org/10.1093/mnrasl/sls021
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society: Letters
Issue: 1
ISSN: 0035-8711