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• W2098546103 abstract "LS I +61 303 is a puzzling object detected from radio up to very high-energy gamma-rays. Variability has recently been observed in its high-energy emission. The object is a binary system, with a compact object and a Be star as primary. The nature of the secondary and the origin of the gamma-ray emission are not clearly established at present. Recent VLBA radio data have been used to claim that the system is a Be /neutron star colliding wind binary, instead of a microquasar. We review the main views on the nature of LS I +61 303 and present results of 3D SPH simulations that can shed some light on the nature of the system. Our results support an accretion powered source, compatible with a microquasar interpretation." @default.
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• W2098546103 date "2008-09-01" @default.
• W2098546103 modified "2023-09-25" @default.
• W2098546103 title "LS I +61 303: MICROQUASAR OR NOT MICROQUASAR?" @default.
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• W2098546103 doi "https://doi.org/10.1142/s0218271808013510" @default.
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