Laboratory Detection of the Carbon Chains HC[TINF]15[/TINF]N and HC[TINF]17[/TINF]N

Michael McCarthy, Jens‐Uwe Grabow, M. J. Travers, W. Chen, C. A. Gottlieb, P. Thaddeus

The Astrophysical Journal · 1998 · 62 citations · 13 references

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Abstract

The linear cyanopolyynes HC15N and HC17N were detected in the laboratory by Fourier transform microwave spectroscopy. Enough rotational lines of each species were measured in the 5-11 GHz frequency range so that precise values for the rotational and centrifugal distortion constants can be determined and the entire rotational spectra of both molecules predicted to better than 1 km s−1 in equivalent radial velocity over the range of interest to radio astronomy. Although there is a nearly constant decrement in line intensity from HC3N to HC9N of about seven, the decrement decreases by at least a factor of 2 on reaching HC17N, and as a result the lines of HC17N are nearly an order of magnitude stronger than predicted by extrapolation from the shorter cyanopolyynes. With a molecular weight of 219 amu and a rotational constant of slightly more than 50 MHz, HC17N is the longest carbon chain identified to date by high-resolution spectroscopy.

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