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Uniform Supersonic Chemical Reactors: 30 Years of Astrochemical History and Future Challenges
Author(s) -
Potapov Alexey,
Canosa André,
Jiménez Elena,
Rowe Bertrand
Publication year - 2017
Publication title -
angewandte chemie international edition
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 5.831
H-Index - 550
eISSN - 1521-3773
pISSN - 1433-7851
DOI - 10.1002/anie.201611240
Subject(s) - astrochemistry , astrobiology , physics , planet , stars , interstellar medium , astronomy , astrophysics , supersonic speed , galaxy , thermodynamics
The interstellar medium is of great interest to us as the place where stars and planets are born and from where, probably, the molecular precursors of life came to Earth. Astronomical observations, astrochemical modeling, and laboratory astrochemistry should go hand in hand to understand the chemical pathways to the formation of stars, planets, and biological molecules. We review here laboratory experiments devoted to investigations on the reaction dynamics of species of astrochemical interest at the temperatures of the interstellar medium and which were performed by using one of the most popular techniques in the field, CRESU. We discuss new technical developments and scientific ideas for CRESU, which, if realized, will bring us one step closer to understanding of the astrochemical history and the future of our universe.

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