The origin of the X-ray-emitting object moving away from PSR B1259–63
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/456/1/L64/8009907/slv171.pdf
Reference13 articles.
1. Modelling interaction of relativistic and non-relativistic winds in binary system PSR B1259−63/SS2883 – I. Hydrodynamical limit
2. Modelling the interaction between relativistic and non-relativistic winds in the binary system PSR B1259−63/SS2883★- II. Impact of the magnetization and anisotropy of the pulsar wind
3. Large-scale flow dynamics and radiation in pulsarγ-ray binaries
4. Simulations of stellar/pulsar-wind interaction along one full orbit
5. Orbital evolution of colliding star and pulsar winds in 2D and 3D: effects of dimensionality, EoS, resolution, and grid size
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1. A Dragon Out of Breath? Monitoring High-velocity Outflows from the High-mass Gamma-Ray Binary LS 2883/PSR B1259–63 During the 2017–2021 Binary Cycle;The Astrophysical Journal;2023-11-01
2. High-resolution simulations of LS 5039;Astronomy & Astrophysics;2023-08-24
3. First Ejection from the PSR B1259-63/LS 2883 High Mass Gamma-Ray Binary Detected During the 2021–2024 Binary Cycle;Research Notes of the AAS;2023-03-14
4. Formation of periodic FRB in binary systems with eccentricity;Monthly Notices of the Royal Astronomical Society;2022-06-13
5. The Major Role of Eccentricity in the Evolution of Colliding Pulsar-Stellar Winds;Universe;2021-07-31
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