Identification of Methyl Isocyanate and Other Complex Organic Molecules in a Hot Molecular Core, G31.41+0.31

G31.41+0.31 is a well known chemically rich hot molecular core (HMC). Using Band 3 observations from the Atacama Large Millimeter Array (ALMA), we have analyzed chemical and physical properties of source. We identified methyl isocyanate (CH3NCO), precursor prebiotic molecules, toward In addition to this, reported presence complex organic molecules (COMs) like methanol (CH3OH), methanethiol (CH3SH), formate (CH3OCHO). Additionally, used transitions HCN, H13CO+, SiO trace infall outflow signatures around star-forming region. For COMs, estimated column densities kinetic temperatures, assuming excitation under local thermodynamic equilibrium (LTE) conditions. From temperatures certain found that multiple temperature components may be present in HMC environment. Comparing obtained between existing observational results other HMCs, it seems COMs are favorably produced environment (?100 K or higher). Though spectral emissions not fully resolved, find CH3NCO possibly formed on grain/ice phase populate gas similar cores Sgr B2, Orion KL, G10.47+0.03.