Abstract
Four new cumulene carbenes, and were detected in the laboratory by H 2 C 7 , H 2 C 8 , H 2 C 9 , D 2 C 10 , Fourier transform microwave spectroscopy. Like the shorter cumulenes in this series, all four were found to have singlet electronic ground states and linear carbon chain backbones. Rotational and centrifugal distortion constants were determined to high accuracy for each molecule, and the entire radio spectrum of each can be calculated to better than 0.3 km s~1 in equivalent radial velocity up to 100 GHz. Upper limits of the and column densities have been estimated for the circumstellar shell of H 2 C 7 , H 2 C 8 , H 2 C 9 the evolved carbon star IRC ]10216. Subject headings : ISM : molecules È line : identiÐcation È molecular data È molecular processes È radio lines : ISM È stars : individual (IRC ]10216)
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CITATION STYLE
Apponi, A. J., McCarthy, M. C., Gottlieb, C. A., & Thaddeus, P. (2000). Laboratory Detection of Four New Cumulene Carbenes: H 2 C 7 , H 2 C 8 , H 2 C 9 , and D 2 C 10. The Astrophysical Journal, 530(1), 357–361. https://doi.org/10.1086/308353
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