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- W1978138745 endingPage "970" @default.
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- W1978138745 abstract "Significance In molecular clouds out of which stars and planetary systems form, simple solid-state molecules made in large part of H 2 O, CO, CO 2 , CH 3 OH, and NH 3 are abundantly present. In these environments, energetic and thermal processes on these ices, which can be simulated in the laboratory, lead to complex organic matter. Possibly at the origin of the organic matter in our Solar System and incorporated into planetesimals, this material may be considered as a potential source for prebiotic chemistry on telluric planets, following a process that may be quite universal. The composition of these laboratory-evolved ices includes potentially prebiotic species such as amino acids and, as presented in this paper, aldehydes and sugars." @default.
- W1978138745 created "2016-06-24" @default.
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- W1978138745 date "2015-01-12" @default.
- W1978138745 modified "2023-10-15" @default.
- W1978138745 title "Aldehydes and sugars from evolved precometary ice analogs: Importance of ices in astrochemical and prebiotic evolution" @default.
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- W1978138745 doi "https://doi.org/10.1073/pnas.1418602112" @default.
- W1978138745 hasPubMedCentralId "https://www.ncbi.nlm.nih.gov/pmc/articles/4313837" @default.
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