Pulse profiles of millisecond pulsars and their Fourier amplitudes

Details Pulse profiles of millisecond pulsars and their Fourier amplitudes Pulse profiles of millisecond pulsars and their Fourier amplitudes

2006-08-30

arxiv.org/abs/astro-ph/0608663v2

Mon.Not.Roy.Astron.Soc.373:836-844,2006

Astronomy and Astrophysics

Astrophysics

9 pages, 6 figures; replaced with the version published in MNRAS

Scientific paper

10.1111/j.1365-2966.2006.11088.x

Approximate analytical formulae are derived for the pulse profile produced by
small hot spots on a rapidly rotating neutron star. Its Fourier amplitudes and
phases are calculated. The proposed formalism takes into account gravitational
bending of light, Doppler effect, anisotropy of emission, and time delays. Its
accuracy is checked with exact numerical calculations.

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