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Current Views on Astrochemistry
1987Astrochemistry is the study of the formation and destruction of interstellar and circumstellar molecules. Such molecules have been a major field of astrophysical investigation for about 17 years. As of 1987 January, 66 species are identified, and the discovery rate is about three per year.
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Recent developments in astrochemistry
AIP Conference Proceedings, 1994I describe the astronomical regions in which chemistry is known to occur, and list the types of molecules that have been positively identified. Some of the successes and failures of chemistries that have been proposed to give rise to these molecular species are reviewed.
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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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Prebiotic Astrochemistry from Astronomical Observations and Laboratory Spectroscopy.
Annual review of physical chemistry (Print)L. Ziurys
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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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Machine learning prediction of state-to-state rate constants for astrochemistry
Artificial Intelligence ChemistryD. Bossion, Gunnar Nyman, Y. Scribano
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