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• W4220702454 endingPage "2017" @default.
• W4220702454 startingPage "2007" @default.
• W4220702454 abstract "As of early 2022, only six species bearing an N-O bond have been detected toward cold molecular clouds and regions of star formation. It is not clear yet if the small number of N-O bond species found in the interstellar medium so far stems from physical and technological limitations of astronomical detection techniques, or whether in fact molecules that bear an N-O bond are for some reason rare in these objects of the interstellar medium. Astronomical N-O bearing molecules are important because they are part of astrochemical models which propose that they are precursors of hydroxylamine (NH2OH), a species linked to the formation of prebiotic amino acids in space. The aim of this study is the better understanding of the open question of the interstellar synthesis of N-O bearing species. We have analyzed by infrared spectroscopy an astrophysically relevant polar ice mixture of N2O:H2O processed by 90 MeV 136Xe23+ ions, which can mimic the physicochemical processes triggered by cosmic rays in water-covered interstellar ice grains. The results show the formation of N2O3 and of H2O2, but no HN-O species of any kind were detected. Such findings are discussed in light of recent studies from our group and from the literature." @default.
• W4220702454 created "2022-04-03" @default.
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• W4220702454 date "2022-03-18" @default.
• W4220702454 modified "2023-10-18" @default.
• W4220702454 title "Infrared Spectroscopic Study on Swift-Ion Irradiation of Solid N₂O–H₂O Samples: Synthesis of N–O Bearing Species in Astrophysical Ices" @default.
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• W4220702454 doi "https://doi.org/10.1021/acs.jpca.2c00768" @default.
• W4220702454 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/35302766" @default.
• W4220702454 hasPublicationYear "2022" @default.
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