Abstract
We present a high-resolution study of a massive dense core JCMT 18354-0649S with the Submillimeter Array. The core is mapped with continuum emission at 1.3 mm, and molecular lines including CHOH (-) and HCN (3-2). The dust core detected in the compact configuration has a mass of and a diameter of $2\arcsec$ (0.06 pc), which is further resolved into three condensations with a total mass of under higher spatial resolution. The HCN (3-2) line exhibits asymmetric profile consistent with infall signature. The infall rate is estimated to be yr. The high velocity HCN (3-2) line wings present an outflow with three lobes. Their total mass is and total momentum is km s, respectively. Analysis shows that the N-bearing molecules especially HCN can trace both inflow and outflow.
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