Results 261 to 270 of about 10,581 (275)
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Interstellar Molecules and Astrochemistry

1988
The quantitative study of the interstellar medium (ISM) began with Hartman’s detection in 1904 of the resonance lines of Ca and K, seen in absorption against bright stars by intervening diffuse clouds. Other atoms (Na,Fe,Ti) were subsequently detected, although the overwhelming abundance of H was not recognized until the 1930s.
Lucy M. Ziurys, Barry E. Turner
openaire   +2 more sources

Computational astrochemistry: general discussion.

Faraday discussions, 2023
Stefan T Bromley   +19 more
semanticscholar   +1 more source

Astrochemistry and compositions of planetary systems

Physics Reports, 2021
Karin I ÖBerg, Edwin A Bergin
exaly  

Astrochemistry

Physical Chemistry Chemical Physics, 2014
openaire   +2 more sources

Hydrogen‐atom tunneling reactions in solid para ‐hydrogen and their applications to astrochemistry

Journal of the Chinese Chemical Society (Taipei), 2022
K. Haupa, P. Joshi, Yuan‐Pern Lee
semanticscholar   +1 more source

Theoretical Chemistry for Astrochemistry

2017
Almost 200 molecules have been detected so far in the interstellar medium and circumstellar shells among which 60 are organic compounds with more than 6 atoms with a straight-chain backbone. Understanding the formation and destruction paths of these molecules both in the gas-phase and in/on solids (cosmic grains, ices) is crucial to diagnose the ...
openaire   +2 more sources

Gas-Phase and Model Ice-Surface Reactions of S(1D) with Water and Methanol: A Computational Investigation and Implications for Cosmochemistry/Astrochemistry

ACS Earth and Space Chemistry
Andrea Giustini   +5 more
semanticscholar   +1 more source

Machine learning prediction of state-to-state rate constants for astrochemistry

Artificial Intelligence Chemistry
D. Bossion, Gunnar Nyman, Y. Scribano
semanticscholar   +1 more source

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