Abstract
We report simultaneous X-ray, optical, and radio observations of V404 Cyg in quiescence. The X-ray flux varied dramatically by a factor of >20 during a 60 ks observation. X-ray variations were well correlated with those in Hα , although the latter include an approximately constant component as well. Correlations can also be seen with the optical continuum, although these are less clear. We see no large lag between X-ray and optical line variations; this implies they are causally connected on short timescales. As in previous observations, Hα flares exhibit a double-peaked profile suggesting emission distributed across the accretion disk. The peak separation is consistent with material extending outward to at least the circularization radius. The prompt response in the entire Hα line confirms that the line variability is powered by X-ray (and/or EUV) irradiation. The origin of the optical continuum variability, whether reprocessing or synchrotron, remains less clear. We also see substantial radio variability at this epoch suggesting sustained outflow of material in quiescence. Chandra observations were supported by NASA grant GO3-4044X.