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

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

2002-05-15

arxiv.org/abs/astro-ph/0205224v1

Astronomy and Astrophysics

Astrophysics

4 pages, 5 Postscript figures, use moriond.sty, latex2e and dvips2e, to apear in the proceedings of the 22nd Moriond Astrophys

Scientific paper

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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