New-wave pulsars

Details New-wave pulsars New-wave pulsars

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987s%26t....73...22w&link_type=abstract

Sky and Telescope (ISSN 0037-6604), vol. 73, Jan. 1987, p. 22-24.

Physics

Accretion Disks, Pulsars, Stellar Magnetic Fields, Stellar Oscillations, Periodic Variations, Power Spectra, Wave Propagation, X Ray Binaries

Scientific paper

The nature of pulsars that exhibit quasi-periodic oscillations (QPOs) is
discussed. It is shown how QPOs are produced by an interaction between
the accretion disk surrounding a neutron star with the neutron star's
magnetic field. The possible relationship between pulsars that exhibit
QPOs and millisecond pulsars is considered.

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