On the formation of polyacetylenes and cyanopolyacetylenes in Titan's atmosphere and their role in astrobiology†
Abstract
This tutorial review compiles recent experimental and theoretical studies on the formation of polyacetylenes (H(C![[triple bond, length as m-dash]](https://www.rsc.org/images/entities/char_e002.gif) C)nH) and cyanopolyacetylenes (H(C
C)nH) and cyanopolyacetylenes (H(C![[triple bond, length as m-dash]](https://www.rsc.org/images/entities/char_e002.gif) C)nCN) together with their
C)nCN) together with their ![[triple bond, length as m-dash]](https://www.rsc.org/images/entities/char_e002.gif) C)nH, CH3(C
C)nH, CH3(C![[triple bond, length as m-dash]](https://www.rsc.org/images/entities/char_e002.gif) C)nCN) as probed under single collision conditions in crossed beam studies via the elementary reactions of ethynyl (CCH) and
C)nCN) as probed under single collision conditions in crossed beam studies via the elementary reactions of ethynyl (CCH) and 
- This article is part of the themed collection: Prebiotic chemistry
 
                



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