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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 3.

(a) TOF spectra recorded at selected laboratory angles (9﹩\mathop{.}\limits^{^\circ }﹩25–34﹩\mathop{.}\limits^{^\circ }﹩25) for the H2 loss channel (m/z = 50) in the 193 nm photodissociation of vinylacetylene (C4H4). Open circles represent the experimental data. The green lines correspond to the best-fit forward-convolution simulations, while the blue and red lines indicate the individual contributions from true H2 loss and dissociative ionization of the H loss channel (m/z = 51), respectively. (b) Center-of-mass translational energy distributions, P(ET), for the H2 loss channel (blue) and the H loss contribution (red) derived from the best-fit simulations. The shaded regions represent the uncertainties in the fits.

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