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- W35763203 abstract "Cygnus X-3 is a well-known microquasar that shows state changes, strong radio emission, hard X-ray/soft X-ray/radio correlations, and relativistic jets. In 2006 after a period of almost four years of quiescence Cyg X-3 transitioned into an active state which included extended quenched emission and several major radio flares (up to 14 Jy). We conducted a large international observing campaign during this activity and we present here some results of our analysis. In this proceedings we will discuss the X-ray spectrum of Cyg X-3 during the major radio flares. We concentrated on the well-established method of studying black hole binary systems known as hardness-intensity diagram (HID) and applied this to Cyg X-3 archival data. In addition, we performed a principal component analysis (PCA) to study the intrinsic variability of the source during a major flare decay. The ramifications of our findings will be discussed." @default.
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- W35763203 date "2010-01-01" @default.
- W35763203 modified "2023-09-23" @default.
- W35763203 title "The nature of the microquasar Cygnus X-3. New multiwavelength observations" @default.
- W35763203 hasPublicationYear "2010" @default.
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