The ab initio rotational constants of the isocyanopolyynes of formulae
HC5N, HC7N, HC9N, and HC11N have been calculated. Their respective va
lues are 1.3925, 0.5653, 0.3111, and 0.1869 GHz, respectively. Inaccur
acies of just a few tenths of 1% may be expected. The recent discovery
of isocyanopolyynes, and the presence of cyanopolyynes in different i
nterstellar clouds allow one to think that the isocyanopolyynes studie
d here may be detected in the near future.