Time-dependent modeling of TeV-detected, young pulsar wind nebulae
نویسندگان
چکیده
منابع مشابه
TeV gamma-rays from the Northern sky pulsar wind nebulae
We estimate the TeV γ-ray fluxes expected from the population of young pulsars in terms of the self-consistent time dependent hadronic-leptonic model for the high energy processes inside the pulsar wind nebulae (PWNe). This radiation model bases on the hypothesis of Arons and collaborators who postulate that leptons are accelerated inside the nebulae as a result of resonant scattering on heavy ...
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D. Volpi∗ a, L. Del Zanna b, E. Amato c, and N. Bucciantini d a bDipartimento di Astronomia e Scienza dello Spazio-Universitá degli Studi di Firenze, Largo E. Fermi, 2, 50125, Firenze, Italy cINAF-Osservatorio Astronomico di Arcetri, Largo E. Fermi 5, 50125, Firenze, Italy dAstronomy Department, University of California at Berkeley, 601 Campbell Hall, Berkeley, CA 94720-3411, USA delia@arcetri....
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The high resolution capabilities of the High Energy Stereoscopic System (HESS) introduced a new era in Gamma-Ray Astronomy, and opens a new window on pulsar wind nebula (PWN) research. A rotationally induced jet (associated with PSR B1509-58) is resolved for the first time in γ-rays, allowing us to trace the particle transport directly, without having the complicating effect of spatially varyin...
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ژورنال
عنوان ژورنال: Journal of High Energy Astrophysics
سال: 2014
ISSN: 2214-4048
DOI: 10.1016/j.jheap.2014.02.001