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We present the results of ALMA observations of dust continuum emission andmolecular rotational lines toward a dense core, MC27 (aka L1521F), which isconsidered to be very close to the first core phase. We revealed thespatial/velocity structures of the core are very complex and and suggest thatthe initial condition of star formation is highly dynamical.

ALMA Observations of a High-density Core, MC27/L1521F in Taurus: Dynamical Gas Interaction at the Possible Site of a Multiple Star Formation