The Synchrotron-based Far-infrared Spectrum of Propargylamine
Propargylamine (HC≡C–CH _2 –NH _2 ), with a triple bond and an amine group, is a nitrogen-bearing organic molecule of astrochemical interest due to its potential role as a precursor to aminoacetonitrile and other complex organic molecules in the ...
Tianhao Hu +4 more
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The most abundant interstellar molecule, molecular hydrogen (H _2 ), is practically invisible in cold molecular clouds. Astronomers typically use carbon monoxide (CO) to trace the bulk distribution and mass of H _2 in our galaxy and many others.
Michael P. Busch
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Chemistry in Extreme Environments: The Mystery of Molecular Complexity in Space. [PDF]
Puzzarini C, Alessandrini S.
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Wavelength-dependent photofragmentation of pyrazine. [PDF]
Payra SS, Thakkar P, Lenka Y, Aravind G.
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Direct observation of organic molecules in asteroid ryugu revealed by high-resolution atomic force microscope. [PDF]
Iwata K +5 more
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Computational investigation of spin-resolved energy landscapes of FeC<sub>4</sub>H<sub>2</sub> <sup>+</sup> and their astrochemical implications. [PDF]
Shajan S, Thirumoorthy K.
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Abiotic formation of nitrile precursors to amino acids and nucleobases in interstellar ice analogues. [PDF]
Wang J +8 more
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Atom Addition Formation of Thionylimide (HNSO) on Interstellar Dust Grains: Chemical Routes Requiring Oxygen and Nitrogen Atom Surface Diffusion. [PDF]
Del Valle JC +6 more
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Nonequilibrium Synthesis of Glycolamide (NH<sub>2</sub>COCH<sub>2</sub>OH), a Precursor to Amino Acids, on Interstellar Nanoparticles. [PDF]
Bergantini A +5 more
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