with a star. The fact that S-2 is unresolved is consistent with this interpretation.

Source A
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This source is clearly resolved. It appears to be part of a diffuse region of emission that connects with the brighter component of the northern lobe. Source A could actually be part of the outflow, either if the outflow is less collimated and the ionized gas preferentially highlights regions where the flow is interacting with dense ambient material or if source A is part of the northern flow being deflected to the east by interaction with a dense clump of gas. The second possibility is interesting and it may be related to the fact that components N1 and N2 are the only ones in the region showing methanol maser emission. It is possible that the methanol maser emission is being stimulated by the deflection of the jet, as it interacts with N1 and N2. Finally, the position of source A could be understood if the outflow has precession (see discussion in Section 5). High angular resolution observations of a tracer of dense molecular gas are needed to advance our understanding of this source.

Source D
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Source D is the faint source located 