The radio to TeV orbital variability of the microquasar LS I +61 303
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20065830/pdf
Reference44 articles.
1. Variable Very-High-Energy Gamma-Ray Emission from the Microquasar LS I +61 303
2. Propagation of very high energy -rays inside massive binaries LS 5039 and LSI +61 303
3. Very-high-energy gamma radiation associated with the unshocked wind of the Crab pulsar
4. γ-ray emission from microquasars: A numerical model for LSI +61°303
5. A broadband leptonic model for gamma-ray emitting microquasars
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1. Owens Valley Radio Observatory monitoring of LS I +61°303 completes three cycles of the super-orbital modulation;Astronomy & Astrophysics;2024-03
2. Achromatic rapid flares in hard X-rays in the γ-ray binary LS I + 61 303;Monthly Notices of the Royal Astronomical Society;2023-08-03
3. Rapid X-ray variability of the gamma-ray binary LS I +61°303;Monthly Notices of the Royal Astronomical Society;2023-06-06
4. Optical microflares in LS I +61 303 and the search for their multiwavelength counterpart;Astronomy & Astrophysics;2022-06
5. A Precessing Jet Scenario for the Multi-Wavelength Long-Term Modulation of LS I +61°303;Universe;2021-07-14
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