Ligterink, Niels F. W. published the artcileThe family of amide molecules toward NGC 6334I, Synthetic Route of 123-39-7, the main research area is amide mol chem network star interstellar dust.
Amide mols. produced in space could play a key role in the formation of biomols. on a young planetary object. However, the formation and chem. network of amide mols. in space is not well understood. In this work, Atacama Large Millimeter/submillimeter Array observations are used to study a number of amide(-like) mols. toward the high-mass star-forming region NGC 6334I. The first detections of cyanamide (NH2CN), acetamide (CH3C(O)NH2), and N-methylformamide (CH3NHCHO) are presented for this source. These are combined with analyses of isocyanic acid (HNCO) and formamide (NH2CHO), and a tentative detection of urea (carbamide; NH2C(O)NH2). Abundance correlations show that most amides are likely formed in related reactions occurring in ices on interstellar dust grains in NGC 6334I. However, in an expanded sample of sources, large abundance variations are seen for NH2CN that seem to depend on the source type, which suggests that the phys. conditions within the source heavily influence the production of this species. The rich amide inventory of NGC 6334I strengthens the case that interstellar mols. can contribute to the emergence of biomols. on planets.
Astrophysical Journal published new progress about Amides Role: TEM (Technical or Engineered Material Use), USES (Uses). 123-39-7 belongs to class amides-buliding-blocks, name is N-Methylformamide, and the molecular formula is C2H5NO, Synthetic Route of 123-39-7.
Referemce:
Amide – Wikipedia,
Amide – an overview | ScienceDirect Topics