Fig. A.1

Example of SED fits to two cores in the active region. Top panel: all flux densities can be fitted with a single greybody; there is no excess at 70 μm, and this core is recognised as a pre-stellar core. The core in the lower panel has an excess flux density at 70 μm (the point has not been excluded from the fit, hence the large χ2). This could be due either to the core being heated from the outside by the FUV radiation field, or to a protostar inside the core (see Sect. 4.2).
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