RCW49 and its ionizing cluster form an extensive, complex region, widely studied at IR and optical wavelengths. Molonglo 843 MHz and ATCA data at 1.4 and 2.4 GHz showed two shells. Recent high-resolution IR imaging revealed a complex dust structure and ongoing star formation. New high-bandwidth and high-resolution data of the RCW49 field were obtained to survey the radio emission at arcsec scale and investigate the small-scale features and nature of the HII region.- Data were collected with the new 2-GHz bandwidth receivers and the CABB correlator of the ATCA, at 5.5 and 9.0 GHz. In addition, archival observations at 1.4 and 2.4 GHz have been re-reduced and re-analyzed, together with optical, IR, X-ray, and gamma-ray observations.- The CABB data result in the most detailed radio continuum images of RCW49 to date. The radio emission closely mimics the near-IR emission observed by Spitzer, showing pillars and filaments. The brightest continuum emission comes from the region known as the bridge. The overall flattish spectral index is consistent with a free-free emission mechanism. However, hints of nonthermal components are also present in the bridge. A jet-like structure surrounded by a bubble feature whose nature is still unclear has been discovered close to the Westerlund~2 core. Two apparent bow shocks and a number of discrete sources have been detected as well in the surroundings of RCW49. We also report on and discuss the possible detection of a H RRL.- The radio results support an association between the cm continuum and molecular emission. The detection of the RRL kinematically favors a RCW49 distance of 6--7 kpc. If the negative spectral indices measured at the bridge are caused by synchrotron emission, we propose a scenario where high-energy emission could be produced. Finally, the newly discovered jet-like structure appears to deserve a detailed study by itself.
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