Detection of interstellar cyanamide (NH$$_{2}$$CN) towards the hot molecular core G10.47$$+$$0.03

In the interstellar medium, amide-type molecules play an important role in formation of prebiotic hot molecular cores or high-mass star-formation regions. The complex amide-related molecule cyanamide (NH $$_{2}$$ CN) is known as one rare which has a major urea CONH ). this paper, we presented detection rotational emission lines towards core G10.47 $$+$$ 0.03 between frequency range 158.49–160.11 GHz using Atacama Large Millimeter/Submillimeter Array (ALMA) interferometric radio telescope. estimated column density NH CN diagram model was $$N(\mathrm{NH}_{2}\mathrm{CN}) = (6.60\pm 0.1)\times 10^{15}$$ cm $$^{-2}$$ with temperature ( $$T_\mathrm{rot}) 201.2\pm 3.3$$ K. fractional abundance respect to H $$f(\mathrm{NH}_{2}\mathrm{CN}) 5.076\times 10^{-8}$$ . Additionally, CN/NH CHO ratio 0.170, nearly similar IRAS 16293–2422 B and Sgr B2 (M). We found that observed 0.03, fairly agrees theoretical value predicted by Garrod (2013). also discussed possible destruction pathways CN.