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ASTROCHEMISTRY: AN UNFINISHED SYMPHONY
Proceedings of the Dalgarno Celebratory Symposium, 2009Alex Dalgarno has introduced many of the themes that define current research in astrochemistry. Variations on these themes will continue to be played out well into the future. Clear and unambiguous tests of theories of formation of interstellar molecules remain elusive; however, the understanding of fluorine chemistry appears to offer one success story.
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Rotational spectroscopy and astrochemistry
Journal of Molecular Structure, 1995Abstract During the last 25 years, the close collaboration between laboratory spectrocopists and astrophysicists allowed the detection of about one hundred different molecular species in the interstellar medium, largely via their rotational emission spectra.
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Recent progress in astrochemistry
Space Science Reviews, 1989Models of the four currently recognized regimes of astrochemistry are compared with observations. Ion-Molecule Gas Phase Chemistry is fundamental throughout all interstellar and circumstellar molecular clouds, and by itself explains fairly well the simpler molecular species in diffuse and cold quiescent dense interstellar clouds, as well as in the ...
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Suprathermal particles in astrochemistry
Russian Chemical Reviews, 2019The kinetic Monte Carlo method, used in astrochemistry to investigate suprathermal (hot) particles at the molecular level, is presented. Different modifications of this method, aimed at studying the influence of suprathermal particles in the processes occurring ...
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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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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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Gas-phase Chemistry in the Interstellar Medium: The Role of Laboratory Astrochemistry
Frontiers in Astronomy and Space Sciences, 2022Cristina Puzzarini
exaly