Ultraviolet photolysis of H2S and its implications for SH radical production in the interstellar medium
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 tha...
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Nature Portfolio
2020
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oai:doaj.org-article:3d3d049e5549412eb63ee6332d1ad8842021-12-02T17:32:42ZUltraviolet photolysis of H2S and its implications for SH radical production in the interstellar medium10.1038/s41467-020-15343-42041-1723https://doaj.org/article/3d3d049e5549412eb63ee6332d1ad8842020-03-01T00:00:00Zhttps://doi.org/10.1038/s41467-020-15343-4https://doaj.org/toc/2041-1723Sulfur 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.Jiami ZhouYarui ZhaoChristopher S. HansenJiayue YangYao ChangYong YuGongkui ChengZhichao ChenZhigang HeShengrui YuHongbin DingWeiqing ZhangGuorong WuDongxu DaiColin M. WesternMichael N. R. AshfoldKaijun YuanXueming YangNature PortfolioarticleScienceQENNature Communications, Vol 11, Iss 1, Pp 1-8 (2020) |
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Science Q |
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Science Q 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 Ultraviolet photolysis of H2S and its implications for SH radical production in the interstellar medium |
description |
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. |
format |
article |
author |
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 |
author_facet |
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 |
author_sort |
Jiami Zhou |
title |
Ultraviolet photolysis of H2S and its implications for SH radical production in the interstellar medium |
title_short |
Ultraviolet photolysis of H2S and its implications for SH radical production in the interstellar medium |
title_full |
Ultraviolet photolysis of H2S and its implications for SH radical production in the interstellar medium |
title_fullStr |
Ultraviolet photolysis of H2S and its implications for SH radical production in the interstellar medium |
title_full_unstemmed |
Ultraviolet photolysis of H2S and its implications for SH radical production in the interstellar medium |
title_sort |
ultraviolet photolysis of h2s and its implications for sh radical production in the interstellar medium |
publisher |
Nature Portfolio |
publishDate |
2020 |
url |
https://doaj.org/article/3d3d049e5549412eb63ee6332d1ad884 |
work_keys_str_mv |
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