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The red MSX source G034.5964-01.0292 (MSXG34), catalogued as a massive YSO,was observed in molecular lines with the aim of discover and study molecularoutflows. We mapped a region of 3'x3' centered at MSXG34 using the AtacamaSubmillimeter Telescope Experiment in the 12CO J=3-2 and HCO+ J=4-3 lines withan angular and spectral resolution of 22" and 0.11 km/s, respectively.Additionally, public 13CO J=1-0 and near-IR UKIDSS data obtained from theGalactic Ring Survey and the WFCAM Sciencie Archive, respectively, wereanalyzed. We found that the 12CO spectra towards the YSO present aself-absorption dip, as it is usual in star forming regions, and spectral wingsevidencing outflow activity. The HCO+ was detected only towards the MSXG34position at v_LSR ~ 14.2 km/s, in coincidence with the 12CO absorption dip andapproximately with the velocity of previous ammonia observations. HCO+ and NH3are known to be enhanced in molecular outflows. Analyzing the spectral wings ofthe 12CO line, we discovered misaligned red- and blue-shifted molecularoutflows associated with MSXG34. The near-IR emission shows a cone-like shapenebulosity composed by two arc-like features related to the YSO, which can bedue to a cavity cleared in the circumstellar material by a precessing jet. Thiscan explain the misalignment in the molecular outflows. From the analysis ofthe 13CO J=1--0 data we suggest that the YSO is very likely related to amolecular clump ranging between 10 and 14 km/s. This suggests that MSXG34, withan associated central velocity of about 14 km/s, may be located in thebackground of this clump. Thus, the blue-shifted outflow is probably deflectedby the interaction with dense gas along the line of sight.

Discovering a misaligned CO outflow related to the red MSX source G034.5964-01.0292