Fig. B.6

SEDs of the members and probably members with IR excess typical of Class I objects, early-type very embedded stars, and uncertain objects within the cloud. 21374388+5734521 is an uncertain case that could be a depleted disk or a combination of two sources. In the case of 214005669+574417181, 214048489+573202607, and 214148062+572609205, the small excess at 8 μm with uncertain photometry does not allow us to determine if they are TD or diskless sources. These sources are not included in the statistics of disk types discussed in the text.
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