A model of two-stream non-radial accretion for binary X-ray pulsars (Q789951)
From MaRDI portal
 | This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: A model of two-stream non-radial accretion for binary X-ray pulsars |
scientific article; zbMATH DE number 3847071
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | A model of two-stream non-radial accretion for binary X-ray pulsars |
scientific article; zbMATH DE number 3847071 |
Statements
A model of two-stream non-radial accretion for binary X-ray pulsars (English)
0 references
1982
0 references
The non-radial accretion is considered in the case of X-ray binary systems. In particular a two-stream model which can be treated as the first approximation of the general problem of a neutron star evolution is introduced. The obtained results are compared with some observational facts regarding the spin time variation for various pulsars.
0 references
non-radial accretion
0 references
X-ray binary systems
0 references
two-stream model
0 references
neutron star evolution
0 references
spin time variation
0 references
pulsars
0 references
