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Photodissociation Pathways of Vinylacetylene (C4H4) and Implications for the Interstellar Hydrocarbon Chemistry

  • Authors: Surajit Metya, Daniel González, Alexander N. Morozov, Alexander M. Mebel, Domenico Stranges, Ralf I. Kaiser

Surajit Metya et al 2026 The Astrophysical Journal 1010 .

  • Provider: AAS Journals

Caption: Figure 5.

TOF spectra recorded at laboratory angles from 9﹩\mathop{.}\limits^{^\circ }﹩25 to 49﹩\mathop{.}\limits^{^\circ }﹩25 for m/z = 25 in the 193 nm photodissociation of vinylacetylene (C4H4). Open circles represent the experimental data. The spectra are reproduced by forward-convolution simulations incorporating contributions from atomic hydrogen loss, molecular hydrogen loss, and the C2H2/CCH2 loss channel. The red, blue, and purple curves denote the individual contributions arising from dissociative ionization of the H loss channel (m/z = 51), the H2 loss channel (m/z = 50), and the true C2H2/CCH2 loss channel, respectively.

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