arxiv: astro-ph/0205224 · v1 · submitted 2002-05-15 · 🌌 astro-ph

The dependence of observed gamma-ray pulsar spectra on viewing geometry

Agnieszka Wozna (1) , Jaroslaw Dyks (1) , Tomasz Bulik (2) , Bronislaw Rudak (1 , 3) ((1) Copernicus Astronomical Center , Torun , Poland , (2) Copernicus Astronomical Center

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Warsaw (3) Dept. of Astronomy Astrophysics of Nicolaus Copernicus University Poland)

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keywords spectraanglesaxisgamma-rayobservedpulsarsrotationviewing

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We calculate the gamma-ray lightcurves and spectra of rotation powered pulsars for a wide range of observer's viewing angles, and inclination angles of the magnetic axis to the rotation axis. We show how the shapes of the observed phase-averaged spectra as well as energy-integrated pulse profiles depend on the orientation for classical and millisecond pulsars.

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The dependence of observed gamma-ray pulsar spectra on viewing geometry

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