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We have analyzed the Atacama Large Millimeter/submillimeter Array (ALMA)cycle 2 data of band 6 toward the G345.4938+01.4677 massive young protostellarobject (G345.5+1.47 MYSO) in the IRAS 16562--3959 high-mass star-forming regionwith an angular resolution of $\sim 0.3"$, corresponding to $\sim 760$ au. Wespatially resolve the central region which consists of three prominentmolecular emission cores. A hypercompact (HC) H$_{\rm {II}}$ region (Core A)and two molecule-rich cores (Core B and Core C) are identified using the momentzero images of the H30$\alpha$ line and a CH$_{3}$OH line, respectively.Various oxygen-bearing complex organic molecules (COMs), such as(CH$_{3}$)$_{2}$CO and CH$_{3}$OCHO, have been detected toward the positions ofCore B and Core C, while nitrogen-bearing species, CH$_{3}$CN, HC$_{3}$N andits $^{13}$C isotopologues, have been detected toward all of the cores. Wediscuss the formation mechanisms of H$_{2}$CO by comparing the spatialdistribution of C$^{18}$O with that of H$_{2}$CO. The $^{33}$SO emission, onthe other hand, shows a ring-like structure surrounding Core A, and it peaks onthe outer edge of the H30$\alpha$ emission region. These results imply that SOis enhanced in a shock produced by the expanding motion of the ionized region.

Chemical composition in the IRAS 16562--3959 high-mass star-forming region