  In this work we present high resolution spectroscopic data of the giant
star-forming region of N11, obtained with the GIRAFFE instrument at the Very
Large Telescope. By using this data set, we find that most of the H$\alpha$
emission lines profiles in this complex can be fitted by a single Gaussian,
however, multiple emission line profiles can be observed in the central region
of N11. By adding all the spectra, we derive the integrated H$\alpha$ profile
of this complex, which displays a width ($\sigma$) of about 12 km s$^{-1}$
(corrected by instrumental and thermal width). We find that a single Gaussian
fit on the integrated H$\alpha$ profile leaves remaining wings, which can be
fitted by a secondary broad Gaussian component. In addition, we find high
velocity features, which spatially correlate with soft diffuse X-ray emission.
