γ-rays from binary system with energetic pulsar and Be star with aspherical wind: PSR B1259−63/SS2883
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/385/4/2279/18237443/mnras0385-2279.pdf
Reference50 articles.
1. Particle acceleration by ultrarelativistic shocks: theory and simulations
2. The Crab Nebula and Pulsar between 500 GeV and 80 TeV: Observations with the HEGRA Stereoscopic Air Cerenkov Telescopes
3. Discovery of the binary pulsar PSR B1259-63 in very-high-energy gamma rays around periastron with HESS
4. Pair formation above pulsar polar caps - Structure of the low altitude acceleration zone
5. Shock Geometry and Inverse Compton Emission from the Wind of a Binary Pulsar
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2. GeV emission of gamma-ray binary with pulsar scenario;Monthly Notices of the Royal Astronomical Society;2020-04-13
3. Evolution of the Extended X-Ray Emission from the PSR B1259–63/LS 2883 Binary in the 2014–2017 Binary Cycle;The Astrophysical Journal;2019-09-04
4. Modelling multiwavelength emissions from PSR B1259–63/LS 2883: Effects of the stellar disc on shock radiations;Astronomy & Astrophysics;2019-07
5. Wind inhibition by X-ray irradiation in HMXBs: the influence of clumping and the final X-ray luminosity;Astronomy & Astrophysics;2018-12
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