Laboratory Detection of the Carbon Chains HC[TINF]15[/TINF]N and HC[TINF]17[/TINF]N
Open Access
- 20 February 1998
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 494 (2) , L231-L234
- https://doi.org/10.1086/311188
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.Keywords
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