Ulsar Model of the High Energy Phenomenology of Ls
نویسنده
چکیده
Under the assumption that LS 5039 is a system composed by a pulsar rotating around an O6.5V star in a ∼ 3.9 day orbit, we present the results of a theoretical modeling of the high energy phenomenology observed by the High Energy Stereoscopy Array (H.E.S.S.). This model (including detailed account of the system geometry, Klein-Nishina inverse Compton, γ-γ absorption, and cascading) is able to describe well the rich observed phenomenology found in the system at all timescales, both flux and spectrum-wise. Subject headings: X-ray binaries (individual LS 5039), γ-rays: observations, γ-rays: theory
منابع مشابه
Model of the High Energy Phenomenology
Under the assumption that LS 5039 is a system composed by a pulsar rotating around an O6.5V star in a ∼ 3.9 day orbit, we present the results of a theoretical modeling of the high energy phenomenology observed by the High Energy Stereoscopy Array (H.E.S.S.). This model (including detailed account of the system geometry, Klein-Nishina inverse Compton, γ-γ absorption, and cascading) is able to de...
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