Several interstellar molecules are highly reactive unsaturated
carbon chains, which are unstable under terrestrial conditions. Laboratory
studies in support of their detection in space thus face the issue
of how to produce these species and how to correctly model their rotational
energy levels. In this work, we introduce a general approach for producing
and investigating unsaturated carbon chains by means of selected test
cases. We report a comprehensive theoretical/experimental spectroscopic
characterization of three species, namely, propadienone, cyanovinylacetylene,
and allenylacetylene, all of them being produced by means of flash
vacuum pyrolysis of a suitable precursor. For each species, quantum-chemical
calculations have been carried out with the aim of obtaining accurate
predictions of the missing spectroscopic information required to guide
spectral analysis and assignment. Rotational spectra of the title
molecules have been investigated up to 400 GHz by using a frequency-modulation
millimeter-/submillimeter-wave spectrometer, thus significantly extending
spectral predictions over a wide range of frequency and quantum numbers.
A comparison between our results and those available in the literature
points out the clear need of the reported laboratory measurements
at higher frequencies for setting up accurate line catalogs for astronomical
searches.