A summary is given of the laboratory study of the rotational spectra of 11
recently detected carbon chain molecules. Classified according to their var
ious end groups, these are the cyanopolyynes HC15N and HC17N; the isocyanop
olyynes HC,NC and HC,NC; the methylcyanopolyynes CH3(C--C)(3)CN, CH3(C drop
C)(4)CN, and CH3(C dropC)(5)CN; and the methylpolyynes CH3(C dropC)(4)H, CH
3(C dropC)(6)H, and CH3(C dropC)(7)H. Measured line frequencies and derived
spectroscopic constants are given for each. The microwave laboratory astro
physics of the entire set is now complete in the sense that all the astrono
mically most interesting rotational transitions, including those with nitro
gen quadrupole hyperfine structure, have now been directly measured or can
be calculated from the derived constants to a small fraction of 1 km s(-1)
in equivalent radial velocity. All 11 carbon chains are candidates for astr
onomical discovery since they are closely related in structure and composit
ion to ones that have already been discovered in space.