Geometry of the emission region of PSR 0950+08

Details Geometry of the emission region of PSR 0950+08 Geometry of the emission region of PSR 0950+08

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...132..312g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 132, no. 2, March 1984, p. 312-316.

Astronomy and Astrophysics

Astrophysics

52

Magnetic Field Configurations, Magnetic Poles, Pulsars, Radio Emission, Stellar Magnetic Fields, Stellar Radiation, Magnetic Dipoles, Microstructure, Stellar Models

Scientific paper

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.

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