Fig. B.9

Overview of the Spitzer spectra (black solid lines) of the carbon-rich PNe with the 30 μm feature. The spectra are ordered according to the Td from high to low temperature, top to bottom, and left to right. They are also normalised to the flux density at 18 μm (in case of SMP LMC 2 it is 18.4 μm) and offset for clarity. The names of objects and values of the Td are shown above spectra.
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