First Astronomical Detection of the Cumulene Carbon Chain Molecule H[TINF]2[/TINF]C[TINF]6[/TINF] in TMC-1

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Abstract
The cumulene carbenes are important components of hydrocarbon chemistry in low-mass star-forming cores. Here we report the first astronomical detection of the long-chain cumulene carbene H2C6 in the interstellar cloud TMC-1, from observations of two of its rotational transitions: JK, K' = 71,7 → 61,6 at 18.8 GHz and 81,8 → 71,7 at 21.5 GHz, using NASA's Deep Space Network 70 m antenna at Goldstone, California. In addition we also observed the shorter cumulene carbene H2C4 at the same position. The fractional abundance of H2C6 relative to H2 is about 4.7 × 10-11 and that of H2C4 is about 1.1 × 10-9. The abundance of H2C6 is in fairly good agreement with gas-phase chemical models for young molecular cloud cores, but the abundance of H2C4 is significantly larger than predicted.
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