Linearly extended cyclotron emission regions in AM Herculis systems

Details Linearly extended cyclotron emission regions in AM Herculis systems Linearly extended cyclotron emission regions in AM Herculis systems

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..405f&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 405-408 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

Cyclotron Radiation, Magnetic Stars, Shock Waves, Stellar Models, Stellar Spectra, Emission Spectra, Light Curve, Polarization Characteristics, Polarized Radiation, Shock Fronts

Scientific paper

The properties of cyclotron radiation originating from homogeneous arc-shaped emission regions are discussed. The effects of field spread across the shock are taken into account. It is found that arc-shaped cyclotron emission regions give rise to asymmetric light and polarization curves which are in closer agreement with observations of some AM Herculis systems than previous point-source and cylindrically extended models.

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