ICREA Workshop on the High Energy Emission from pulsars and their ...
ICREA Workshop on the High Energy Emission from pulsars and their ...
ICREA Workshop on the High Energy Emission from pulsars and their ...
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Unidentified gamma-ray sources:PWNe Sync/IC emissi<strong>on</strong>?(Pellizz<strong>on</strong>i et al., 2005, 2009)PWNe are a comm<strong>on</strong> phenomen<strong>on</strong> associated to young <strong>and</strong> energetic<strong>pulsars</strong> (but weaker than pulsed emissi<strong>on</strong> at GeV).If <strong>the</strong> pulsar beamed emissi<strong>on</strong> does not intersect <strong>the</strong> line of sightto <strong>the</strong> observer, <strong>the</strong> PWN comp<strong>on</strong>ent unhindered by <strong>the</strong> str<strong>on</strong>gerpulsed emissi<strong>on</strong>, could be detectable.E>100 MeVBrightest “undisturbed” <strong>pulsars</strong> = a class of unidentified sources(A new significant comp<strong>on</strong>ent for <strong>the</strong> diffuse gamma-ray emissi<strong>on</strong>?)
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