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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Infrared intensities and molar refraction of amorphous dimethyl carbonate - comparisons to four interstellar molecules. [PDF]
Hudson RL, Coleman FM.
europepmc +1 more source
From the laboratory to the interstellar medium: a strategy to search for exotic molecules in space [PDF]
Cristina Puzzarini +4 more
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Pathways to Oxygen‐Bearing Molecules in the Interstellar Medium and in Planetary Atmospheres: Cyclopropenone (c‐C3H2O) and Propynal (HCCCHO) [PDF]
Li Zhou +5 more
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Discovery of the interstellar chiral molecule propylene oxide (CH 3 CHCH 2 O) [PDF]
Brett A. McGuire +6 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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Observations of Interstellar Molecules with the International Ultraviolet Explorer [PDF]
J. H. Black
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Theoretical studies of interstellar molecular shocks - VI. The formation of molecules containing two or three carbon atoms [PDF]
G. Pineau des Forêts +3 more
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Ultraviolet Observations of Interstellar Molecules [PDF]
Theodore P. Snow
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Laboratory investigation of ion-molecule reactions of HC3N in dense interstellar clouds [PDF]
C. G. Freeman +2 more
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