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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 2.

(a) TOF spectra recorded at selected laboratory angles (9﹩\mathop{.}\limits^{^\circ }﹩25, 14﹩\mathop{.}\limits^{^\circ }﹩25, and 19﹩\mathop{.}\limits^{^\circ }﹩25) for the H loss channel (m/z = 51) in the 193 nm photodissociation of vinylacetylene (C4H4). Open circles represent the experimental data, while the red lines correspond to the best-fit forward-convolution simulations using a single-channel model. (b) Center-of-mass translational energy distribution, P(ET), derived from the best-fit simulation. The shaded region indicates the uncertainty range in the fit.

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