ALMA Observations of a High-density Core, MC27/L1521F in Taurus:
  Dynamical Gas Interaction at the Possible Site of a Multiple Star Formation
  We present the results of ALMA observations of dust continuum emission and
molecular rotational lines toward a dense core, MC27 (aka L1521F), which is
considered to be very close to the first core phase. We revealed the
spatial/velocity structures of the core are very complex and and suggest that
the initial condition of star formation is highly dynamical.
