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• W2024331869 abstract "Using Compton Gamma Ray Observatory BATSE hard X-ray (HXR) data and GHz radio monitoring data from the Green Bank Interferometer, we have performed a long-term study (~1800 days) of the unusual X-ray binary Cyg X-3, resulting in the discovery of a remarkable relationship between these two wavelength bands. We find that during quiescent radio states, the radio flux is strongly anticorrelated with the intensity of the HXR emission. The relationship switches to a correlation with the onset of major radio flaring activity. During major radio flaring activity, the HXR drops to a very low intensity during quenching in the radio and recovers during the radio flare. Injection of plasma into the radio jets of Cyg X-3 occurs during changes in the HXR emission and suggests that disk-related and jet-related components are responsible for the high energy emission." @default.
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• W2024331869 date "1999-06-01" @default.
• W2024331869 modified "2023-10-16" @default.
• W2024331869 title "Discovery of Correlated Behavior between the Hard X‐Ray and the Radio Bands in Cygnus X‐3" @default.
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• W2024331869 doi "https://doi.org/10.1086/307241" @default.
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