Laborastrophysikgruppe des Max-Planck-Instituts für Astronomie am Institut für Festkörperphysik, Friedrich-Schiller-Universität Jena, Helmholtzweg 3, 07743, Jena, Germany.
Département de Physique Moléculaire, Institut de Physique de Rennes, UMR CNRS-UR1 6251, Université de Rennes 1, Campus de Beaulieu, 263 Avenue du Général Leclerc, 35042, Rennes Cedex, France.
Angew Chem Int Ed Engl. 2017 Jul 17;56(30):8618-8640. doi: 10.1002/anie.201611240. Epub 2017 Jun 13.
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.
星际介质是我们非常感兴趣的，因为它是恒星和行星诞生的地方，而且可能是生命的分子前体来到地球的地方。天文观测、天体化学模型和实验室天体化学应该携手合作，以了解恒星、行星和生物分子形成的化学途径。在这里，我们回顾了实验室实验，这些实验致力于研究星际介质温度下天体化学感兴趣的物种的反应动力学，这些实验是使用该领域最流行的技术之一 CRESU 进行的。我们讨论了 CRESU 的新的技术发展和科学思想，如果实现的话，将使我们更接近理解天体化学的历史和我们宇宙的未来。
