G010.32−00.15 at different wavelengths, showing the bipolar nature of the H ii region. The red contours correspond to the column density showing the dust clumps encircling the waist of the nebula (levels of 1.5, 1.0, 0.75, and 0.5 × 10²³ cm^-2). The underlying grey images are a) the VLA radio-continuum image at 21 cm; b) the MIPSGAL map at 24 μm; and c) the PACS map at 70 μm (all in logarithmic units to enhance the diffuse emission regions, especially the two ionized lobes).