How Interstellar Chemistry (and Astrochemistry More Generally) Became Useful

T. Hartquist, S. Loo, S. Falle
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Abstract

In 1986 Alex Dalgarno published a paper entitled "Is Interstellar Chemistry Useful?" By the middle 1970s, and perhaps even earlier, Alex had hoped that astronomical molecules would prove to: possess significant diagnostic utility; control many of the environments in which they exist; stimulate a wide variety of physicists and chemists who are at least as fascinated by the mechanisms forming and removing the molecules as by astronomy. His own research efforts have contributed greatly to the realization of that hope. This paper contains a few examples of: how molecules are used to diagnose large-scale dynamics in astronomical sources including star forming regions and supernovae; the ways in which molecular processes control the evolution of astronomical objects such as dense cores destined to become stars and very evolved giant stars; theoretical and laboratory investigations that elucidate the processes producing and removing astronomical molecules and allow their detection.
星际化学(以及更普遍的天体化学)是如何变得有用的
1986年,亚历克斯·达尔加诺发表了一篇题为《星际化学有用吗?》到20世纪70年代中期,甚至更早的时候,亚历克斯希望天文分子能够证明:具有重要的诊断功能;控制它们存在的许多环境;激发各种各样的物理学家和化学家,他们对分子形成和去除的机制至少像对天文学一样着迷。他自己的研究努力为实现这一希望做出了巨大贡献。本文包含了几个例子:如何使用分子来诊断包括恒星形成区和超新星在内的天文来源中的大规模动力学;分子过程控制天体演化的方式,比如注定要成为恒星的致密核和非常演化的巨星;天体物理学理论和实验室研究,阐明产生和移除天体分子的过程,并允许对其进行探测。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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