MODELING THE RISE OF FIBRIL MAGNETIC FIELDS IN FULLY CONVECTIVE STARS (2016)
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/10.3847/0004-637x/827/2/95
Publication URI: http://dx.doi.org/10.3847/0004-637x/827/2/95
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2