Geometry of the emission region of PSR 0950+08.
Abstract
The geometry of the radio-emission region of PSR 0950+08 is studied. The considerations are based on the estimation of the value of the angle θ between the rotation and magnetic axis and the angle ξ between the magnetic axis and the line-of-sight obtained by Narayan and Vivekanand (1982) and on the observed separation of the main profile components.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- March 1984
- Bibcode:
- 1984A&A...132..312G
- Keywords:
-
- Magnetic Field Configurations;
- Magnetic Poles;
- Pulsars;
- Radio Emission;
- Stellar Magnetic Fields;
- Stellar Radiation;
- Magnetic Dipoles;
- Microstructure;
- Stellar Models;
- Astrophysics