Image Details

Choose export citation format:

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 4.

(a) TOF spectra recorded at laboratory angles from 9﹩\mathop{.}\limits^{^\circ }﹩25 to 49﹩\mathop{.}\limits^{^\circ }﹩25 for the C2H2/CCH2 loss channel (m/z = 26) in the 193 nm photodissociation of vinylacetylene (C4H4). Open circles represent the experimental data. The green dotted line corresponds to the best-fit forward-convolution simulation, while the red, blue, and purple curves (solid lines) denote the individual contributions from dissociative ionization of the H loss channel (m/z = 51), H2 loss channel (m/z = 50), and the true C2H2/CCH2 loss channel, respectively. (b) Center-of-mass translational energy distributions, P(ET), for the H loss (red), H2 loss (blue), and C2H2/CCH2 loss (purple) channels derived from the best-fit simulations. The shaded regions indicate the uncertainties in the fits.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse