Abstract
We present preliminary results of an observation of Cygnus X-1 with INTEGRAL performed on June 711 2003. Both spectral and variability properties of the source indicate that Cygnus X-1 was in an intermediate state. As expected during state transitions, we find an anticorrelation between the 3-10 keV and the 15 GHz radio fluxes and a strong correlation between the 3-200 keV hardness and radio flux.
| Original language | English |
|---|---|
| Pages (from-to) | 341-344 |
| Number of pages | 4 |
| Journal | European Space Agency, (Special Publication) ESA SP |
| Issue number | 552 |
| Publication status | Published - 1 Dec 2004 |
| Externally published | Yes |
| Event | 5th INTEGRAL Workshop on The INTEGRAL Universe - Munich, Germany Duration: 16 Feb 2004 → 20 Feb 2004 |
Keywords
- Black holes
- Gamma-rays
- Individual: Cyg X-1
- X-ray binaries
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