Detection of Circular Polarization in the Galactic Center

We report here the detection of circular polarization in the Galactic Center black hole candidate, Sagittarius A*. The detection was made at 4.8 GHz and 8.4 GHz with the Very Large Array. We nd that the fractional circular polarization at 4.8 GHz is m c = ?0:36 0:05% and that the spectral index of the circular polarization is = ?0:6 0:3 (m c /). The systematic error in m c is less than 0.04% at both frequencies. In light of our recent lower limits on the linear polarization in Sgr A*, this detection is diicult to interpret with standard models. We consider brieey whether scattering mechanisms could produce the observed polarization. Detailed modeling of the source and the scattering medium is necessary. We propose a simple model in which low energy electrons reduce linear polarization through Faraday depolarization and convert linear polarization into circular polarization. Circular polarization may represent a signiicant new parameter for studying the obscured centimeter wavelength radio source in Sgr A*.