Laboratory Detection of the Ring-Chain Molecule C[TINF]7[/TINF]H[TINF]2[/TINF]
Open Access
- 10 July 1997
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 483 (2) , L139-L142
- https://doi.org/10.1086/310748
Abstract
Following the recent laboratory detection of the ring-chain carbene C5H2, we have now detected C7H2, the next longer member of the sequence formed by substituting a carbon chain for one of the hydrogen atoms of cyclic C3H2. The strongest lines, again obtained with a diacetylene-neon discharge, were roughly 15 times weaker than those of C5H2. Enough rotational lines were detected in both the normal and doubly deuterated isotopic species to be certain of the identification and to obtain the rotational and leading centrifugal distortion constants accurately enough for calculation of the entire rotational spectrum below 300 GHz to a fraction of 1 km s-1 in equivalent radial velocity. The ring chain here is calculated to be the most stable isomer of C7H2 and extremely polar, so it is of considerable astronomical interest. Several other isomers of C7H2 may be detectable in the laboratory and in space with present techniques.Keywords
This publication has 15 references indexed in Scilit:
- First Astronomical Detection of the Cumulene Carbon Chain Molecule H[TINF]2[/TINF]C[TINF]6[/TINF] in TMC-1The Astrophysical Journal, 1997
- Electronic spectrum of C6H: in the gas-phase detected by cavity ringdownChemical Physics Letters, 1997
- Structure of the CCCN and CCCCH radicals: Isotopic substitution and ab initio theoryThe Journal of Chemical Physics, 1995
- The interstellar gas phase production of highly complex hydrocarbons: construction of a modelInternational Journal of Mass Spectrometry and Ion Processes, 1995
- The singlet with a C3 ring: the probable candidate of HC6N and C7H2Journal of Molecular Structure: THEOCHEM, 1994
- Most stable isomer and singlet—triplet energy separation in the HC4N moleculeChemical Physics Letters, 1993
- A spectral-line survey of W51 from 17.6 to 22.0 GHzThe Astrophysical Journal Supplement Series, 1993
- A survey of cyclopropenylidene (C3H2) in Galactic sourcesThe Astronomical Journal, 1989
- Gas-phase production of complex hydrocarbons, cyanopolyynes, and related compounds in dense interstellar cloudsThe Astrophysical Journal Supplement Series, 1989
- Origin of diffuse interstellar linesNature, 1977