2005ApJ...633..218B

We report the discovery of a transient radio source 2".7 (0.1 pc projected distance) south of the Galactic center massive black hole, Sgr A*. The source flared with a peak of at least 80 mJy in 2004 March. The source was resolved by the Very Large Array into two components with a separation of ∼0".7 and characteristic sizes of ∼0".2. The two components of the source faded with a power-law index of 1.1±0.1. We detect an upper limit to the proper motion of the eastern component of ∼3x10³ km/s relative to Sgr A*. We detect a proper motion of ∼10⁴ km/s for the western component relative to Sgr A*. The transient was also detected at X-ray wavelengths with the Chandra X-Ray Observatory and XMM-Newton and given the designation CXOGC J174540.0-290031. The X-ray source falls in between the two radio components. The maximum luminosity of the X-ray source is ∼10³⁶ ergs/s, significantly sub-Eddington. The radio jet flux density predicted by the X-ray/radio correlation for X-ray binaries is orders of magnitude less than the measured flux density. We conclude that the radio transient is the result of a bipolar jet originating in a single impulsive event from the X-ray source and interacting with the dense interstellar medium of the Galactic center.