SOLUTION TO THE SIGMA PROBLEM OF PULSAR WIND NEBULAE (2014)
Attributed to:
Dynamics of Relativistic Magnetized Flows.
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1142/s2010194514601689
Publication URI: http://dx.doi.org/10.1142/s2010194514601689
Type: Journal Article/Review
Parent Publication: International Journal of Modern Physics: Conference Series