Axially symmetric relativistic MHD simulations of Pulsar Wind Nebulae in Supernova Remnants. On the origin of torus and jet-like features (Q63411173)
Jump to navigation
Jump to search
scientific article
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Axially symmetric relativistic MHD simulations of Pulsar Wind Nebulae in Supernova Remnants. On the origin of torus and jet-like features |
scientific article |
Statements
29 June 2004
0 references
3
0 references