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

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dc.creatorWozna, Agnieszka
dc.creatorDyks, Jaroslaw
dc.creatorBulik, Tomasz
dc.creatorRudak, Bronislaw
dc.date2002-05-15
dc.date.accessioned2026-07-07T02:03:39Z
dc.date.available2026-07-07T02:03:39Z
dc.descriptionWe 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.
dc.description4 pages, 5 Postscript figures, use moriond.sty, latex2e and dvips2e, to apear in the proceedings of the 22nd Moriond Astrophysics Meeting, Les Arcs 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0205224
dc.identifierhttp://arxiv.org/abs/astro-ph/0205224
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4462
dc.subjectAstrophysics
dc.titleThe dependence of observed gamma-ray pulsar spectra on viewing geometry
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