Nature Communications (Mar 2020)

Ultraviolet photolysis of H2S and its implications for SH radical production in the interstellar medium

  • Jiami Zhou,
  • Yarui Zhao,
  • Christopher S. Hansen,
  • Jiayue Yang,
  • Yao Chang,
  • Yong Yu,
  • Gongkui Cheng,
  • Zhichao Chen,
  • Zhigang He,
  • Shengrui Yu,
  • Hongbin Ding,
  • Weiqing Zhang,
  • Guorong Wu,
  • Dongxu Dai,
  • Colin M. Western,
  • Michael N. R. Ashfold,
  • Kaijun Yuan,
  • Xueming Yang

DOI
https://doi.org/10.1038/s41467-020-15343-4
Journal volume & issue
Vol. 11, no. 1
pp. 1 – 8

Abstract

Read online

Sulfur is abundant in the Universe, but the observed abundance ratio of SH to H2S doesn’t agree with astrochemical models. The authors measure product state-resolved translational energy spectra of photoproducts in a jet-cooled H2S beam as a function of wavelength, showing that SH yield is lower than assumed in the models.