Results 261 to 270 of about 10,581 (275)
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Interstellar Molecules and Astrochemistry
1988The 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
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Computational astrochemistry: general discussion.
Faraday discussions, 2023Stefan T Bromley+19 more
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Astrochemistry and compositions of planetary systems
Physics Reports, 2021Karin I ÖBerg, Edwin A Bergin
exaly
Hydrogen‐atom tunneling reactions in solid para ‐hydrogen and their applications to astrochemistry
Journal of the Chinese Chemical Society (Taipei), 2022K. Haupa, P. Joshi, Yuan‐Pern Lee
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Theoretical Chemistry for Astrochemistry
2017Almost 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 ...
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Machine learning prediction of state-to-state rate constants for astrochemistry
Artificial Intelligence ChemistryD. Bossion, Gunnar Nyman, Y. Scribano
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Astrochemistry: The study of chemical processes in space.
Life sciences and space researchA. Das
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Photochemistry and Astrochemistry: Photochemical Pathways to Interstellar Complex Organic Molecules
Chemical Reviews, 2016Karin I ÖBerg
exaly