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We combine multifrequency observations from the millimeter to near infraredwavelengths that demonstrate the spatial distributions of H2, CO, and NH3emission, which are all manifestations of various shocks driven by outflows ofdeeply embedded sources in NGC6334I. In addition to the well-knownnortheast-southwest outflow we detect at least one more outflow in the regionby combining observations from APEX, ATCA, SMA, Spitzer and VLT/ISAAC.Potential driving sources will be discussed. NGC6334I exhibits several signs ofactive star formation and will be a major target for future observatories suchas Herschel and ALMA.

Synergy of multifrequency studies from observations of NGC6334I