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We present a possible identification strategy for first hydrostatic core(FHSC) candidates and make predictions of ALMA dust continuum emission mapsfrom these objects. We analyze the results given by the different bands andarray configurations and identify which combinations of the two represent ourbest chance of solving the fragmentation issue in these objects. If themagnetic field is playing a role, the emission pattern will show evidence of apseudo-disk and even of a magnetically driven outflow, which purehydrodynamical calculations cannot reproduce.

Simulated ALMA observations of collapsing low-mass dense cores