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- W2755149035 abstract "An understanding of possible scenarios for the formation of astrophysically relevant molecules, particularly complex organic molecules, will bring us one step closer to the understanding of our astrochemical heritage. In this context, formaldehyde is an important molecule as a precursor of methanol, which in turn is a starting point for the formation of more complex organic species. In the present experiments, for the first time, following the synthesis of CO, formaldehyde has been produced on the surface of interstellar grain analogs, hydrogenated fullerene-like carbon grains, by O and H atom bombardment. The formation of H2CO is an indication for a possible methanol formation route in such systems." @default.
- W2755149035 created "2017-09-25" @default.
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- W2755149035 date "2017-09-11" @default.
- W2755149035 modified "2023-10-18" @default.
- W2755149035 title "The Formation of Formaldehyde on Interstellar Carbonaceous Grain Analogs by O/H Atom Addition" @default.
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- W2755149035 doi "https://doi.org/10.3847/1538-4357/aa85e8" @default.
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