Abstract
We report on the first detection of a quasi-simultaneous radio-X-ray flare of Cygnus X-1. The detection was made on 2005 April 16 with pointed observations by the RXTE and the Ryle telescope, during a phase where the black hole candidate was close to a transition from its soft state to its hard state. The radio flare lagged the X-rays by ∼7 minutes, peaking at 3:20 hr barycentric time (TDB 2,453,476.63864). We discuss this lag in the context of models explaining such flaring events as the ejection of electron bubbles emitting synchrotron radiation.
| Original language | English |
|---|---|
| Pages (from-to) | L97-L100 |
| Journal | Astrophysical Journal |
| Volume | 663 |
| Issue number | 2 II |
| DOIs | |
| State | Published - Jul 10 2007 |
Keywords
- Accretion, accretion disks
- Black hole physics
- X-rays: binaries
- X-rays: stars
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