Solution to the Sigma-Problem of Pulsar Wind Nebulae (2012)

First Author: Porth O

Attributed to: Dynamics of Relativistic Magnetized Flows. funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1212.1382

Publication URI: https://arxiv.org/abs/1212.1382

Type: Other