Experimental VUV Photoionization of C<sub>70</sub> and Vibrationally Resolved Spectra of the Excited Electronic States of the C<sub>70</sub> <sup><b>+</b></sup> Cation. [PDF]
Ganner L +6 more
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Time-resolved X-ray spectroscopy of phenanthridine: elucidating the photodynamics of a nitrogen-containing polycyclic aromatic hydrocarbon. [PDF]
Schaffner D +18 more
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Preliminary Prediction of Potential Hepatoprotective Properties of Jujube Extract in Rats Using Metabolomics and Bioinformatics. [PDF]
Liu M +5 more
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Dicyanoacetylene (NC<sub>4</sub>N) Formation in the CN + Cyanoacetylene (HC<sub>3</sub>N) Reaction: A Combined Crossed-Molecular Beams and Theoretical Study. [PDF]
Valença Ferreira de Aragão E +8 more
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The Mechanism and Kinetics of the O(<sup>1</sup>D) + Ethylene Reaction: Effects of a Submerged Peak Induced by van der Waals Interactions. [PDF]
Huang X +5 more
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Laboratory detection and rotational spectroscopy of <i>trans</i>-HNSO: implications for astronomical observations. [PDF]
Lattanzi V +4 more
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Electronic energy transfer ionization in naphthalene-CO2 clusters reveals excited states of dry ice. [PDF]
Lemmens AK +3 more
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© 2021 American Chemical Society.
Olivia Harper Wilkins, Geoffrey A. Blake
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Ever wondered if the chemical processes taking place in space could be related to the origins of life? The authors of this book, both experienced astrochemists, embark on a discussion to find the answers to this question and more, and include a general introduction to astrochemistry for chemistry students.
David A Williams +1 more
exaly +3 more sources
Astronomers have identified some 70 molecular species in dense interstellar clouds and the envelopes expelled by evolved stars. Some 75% of these are organic, including molecules with up to 13 atoms and with weights up to 147 daltons. Elements found in interstellar compounds include H, C, N, O, S, Si, and probably Cl.
Irvine, William M., Hjalmarson, Ake
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