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Fig. A.2


Spectral energy distribution for the relevant sources detected also both at 70 and 24 μm with MIPS (A1 group). Completeness and detection limits have been included for Spitzer data, as gray and black line segments, respectively. For comparison, we have overplotted in the SED panel the expected emission of a 3 Myr object with 0.072 M at the distance of B30 –400pc, without interstellar absorption and with a value of AV = 10 magnitudes (black solid lines).

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