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Radio and optical observations of the PSR B1259–63/SS 2883 Be star binary system

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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1994-05-15 and is currently open access. It has received 151 citations till now. The article focuses on the topics: X-ray binary & X-ray pulsar.

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Gamma-ray binaries : pulsars in disguise?

TL;DR: In this paper, the authors investigate whether the interaction of relativistic wind from a young pulsar with the wind from its stellar companion, as in PSR B1259-63, constitutes a viable scenario for explaining the observations of LS 5039 and LSI+61°303.
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Theory of high-energy emission from the pulsar/Be star system PSR 1259-63. I. Radiation mechanisms and interaction geometry

TL;DR: In this paper, the physical processes in the system containing the 47 ms radio pulsar PSR B1259{minus}63 orbiting around a Be star in a highly eccentric orbit were studied.
Journal ArticleDOI

Gamma-ray binaries and related systems

TL;DR: Gamma-ray binaries are a class of sources of high-energy gamma-ray emissions as discussed by the authors, and they have been shown to be driven by rotation-powered pulsars.
Journal ArticleDOI

High-mass X-ray binaries in the Milky Way

TL;DR: In this paper, the authors classified the super-giant systems into three categories: classical/obscured, eccentric and fast transient, and proposed a model to simulate the accretion process on relatively large scales, including wind clumps, magnetic fields, neutron star rotation and eccentricity.
Journal ArticleDOI

Discovery of high-energy gamma-ray emission from the binary system PSR B1259–63/LS 2883 around periastron with Fermi

A. A. Abdo, +201 more
TL;DR: In this paper, the authors reported the discovery of 100 MeV γ -rays from the binary system PSR B1259−63/LS 2883 using the Large Area Telescope (LAT) on board Fermi.
Related Papers (5)

Discovery of the Binary Pulsar PSR B1259-63 in Very-High-Energy Gamma Rays around Periastron with H.E.S.S

Felix Aharonian, +107 more