HST/WFPC2 Images of the GG Tauri Circumbinary Disk

We present the first visible wavelength images of the GG Tauri circumbinary ring, obtained with the Hubble Space Telescope’s Wide Field and Planetary Camera 2. Scattered light from the ring is detected in both V and I band images. The images show that the ring is smooth, except for a small gap that could be a shadow caused by material between the stars and the ring. The spokes seen extending from the stars to the ring in ground-based adaptive optics images are not seen in our data, which suggests that they may be image artifacts. The nearside/farside surface brightness ratio is 6.9 in I band, consistent with forward scattering by small dust grains. The azimuth of the peak ring surface brightness appears offset by 13 from the azimuth closest to us, as seen in previous nearIR HST observations. This may indicate that the ring is warped or somehow shadowed by the circumstellar disks. The color of the ring is redder than the combined light from the stars as observed by HST, confirming previous measurements that indicate that circumstellar disks may introduce extinction of light illuminating the ring. We detect a bright, compact arc of material 0. 3 from the secondary star at an azimuth opposite the primary. It appears to be too large to be a circumstellar disk and is not at the expected location for dust trapped at a Lagrange point. Subject headings: stars: circumstellar matter — stars: individual (GG Tauri) — stars: pre-main sequence — stars:binaries Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218 ([email protected]) MS 183-900, Jet Propulsion Laboratory, Pasadena, CA 91109 ([email protected]) Instituto de Astronomia, Universidad Nacional Autónoma de México, Apartado Postal 72-3, 58089 Morelia, Michoacán, México ([email protected])