Magnetic inverse Compton scattering above polar caps.

Details Magnetic inverse Compton scattering above polar caps. Magnetic inverse Compton scattering above polar caps.

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...301..456c&link_type=abstract

Astronomy and Astrophysics, v.301, p.456

Astronomy and Astrophysics

Astrophysics

16

Radiation Mechanisms: Non Thermal, Pulsars: General, X-Rays: Stars

Scientific paper

Following Kundt & Schaaf (1993), it is shown that under certain conditions, inverse Compton scattering is the dominant mechanism for braking escaping charges above polar caps rather than the usually invoked curvature radiation. These conditions are: (i) the polar-cap temperature is that indicated by X-rays from PSRs and (ii) either γ

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