Image adapted from [51] showing the H emission profile of the LV2 proplyd observed with FLAMES with an effective velocity resolution of about 2.3 (FWHM velocity resolution of 7.7 ). The red- and blue-shifted components of the bipolar jet are clearly resolved, even without subtracting the bright background emission of the nebula. The intensity scale is logarithmic with a minimum of (black) and a maximum of (white). The length of the vertical axis is .
