Abstract
We present the results of an INTEGRAL observation of Cygnus X-1 in an intermediate state. During our 4 days long observation, the source exhibited a strong flux and spectral variability correlated with the radio emission. The study of this broad band variability suggests that the source made a mini-state transition from a nearly hard state to a nearly soft state, and back.
| Original language | English |
|---|---|
| Pages (from-to) | 345-348 |
| Number of pages | 4 |
| Journal | European Space Agency, (Special Publication) ESA SP |
| Issue number | 622 SP |
| Publication status | Published - 1 Jul 2006 |
| Externally published | Yes |
| Event | 6th Integral Workshop - The Obscured Universe - Moscow, Russian Federation Duration: 2 Jul 2006 → 8 Jul 2006 |
Keywords
- Black hole physics
- Gamma-rays: observations
- Radiation mechanisms: non-thermal
- X-rays: binaries; radio continuum: stars
- X-rays: individual: Cygnus X-1
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