The story of the identification of magnesium isocyanide (MgNC) began with a report by
Guélin et al.
in 1986 of three doublet lines in the circumstellar envelope
IRC+10216. They were unable to match them
to any known species. In 1993,
Kawaguchi et al.
published laboratory data for MgNC. Its rotational spectrum matched the unidentified lines. Theoretical work by
Ishii et al.
helped to confirm the assignment.
MgNC is an unstable radical species. It has a fairly
large dipole moment, which contributes toward its
observability in the molecular clouds via rotational spectroscopy.