SIMBAD references

This work presents a detailed analysis of the laboratory and astrophysical spectral data available for ²⁸SiC₂, ²⁹SiC₂, ³⁰SiC₂, Si¹³CC, and Si₂C. New data on the rotational lines of these species between 70 and 350GHz have been obtained with high spectral resolution (195kHz) with the IRAM 30m telescope in the direction of the circumstellar envelope IRC +10216. Frequency measurements can reach an accuracy of 50kHz for features observed with a good signal to noise ratio. From the observed astrophysical lines and the available laboratory data new rotational and centrifugal distortion constants have been derived for all the isotopologues of SiC₂, allowing us to predict their spectrum with an estimated accuracy better than 50kHz below 500GHz and around 50-100kHz for the strong lines above 500GHz. Improved rotational and centrifugal distortion constants have also been obtained for disilicon carbide, Si₂C. This work shows that observations of IRC +10216 taken with the IRAM 30m telescope, with a spectral resolution of 195kHz, can be used for any molecular species detected in this source to derive, or improve, its rotational constants. Hence, IRC +10216 in addition to be one the richest sources in molecular species in the sky, can also be used as a spectroscopy laboratory in the millimetre and submillimetre domains.