THE CHEMISTRY OF ASTRONOMICAL ENVIRONMENTS

被引：41

作者：

DALGARNO, A

机构：

来源：

JOURNAL OF THE CHEMICAL SOCIETY-FARADAY TRANSACTIONS | 1993年 / 89卷 / 13期

关键词：

D O I：

10.1039/ft9938902111

中图分类号：

O64 [物理化学（理论化学）、化学物理学];

学科分类号：

070304 ; 081704 ;

摘要：

Beginning with the chemistry of the early Universe, a review is presented of the chemistry of astronomical environments beyond the solar system with a particular emphasis on the interstellar medium. The ion-molecule chemistry of a quiescent interstellar cloud is summarized and modifications arising from intense radiation fields and shocks associated with star formation are discussed. The influence of grain chemistry is noted. The formation of molecules in the ejecta of Supernova 1987A is described. The fundamental role of chemistry in stellar and galactic formation and evolution is emphasized.

引用

页码：2111 / 2117

页数：7

共 105 条

[1] VELOCITY STRUCTURE IN OPTICAL CH+ LINES TOWARD HD-190603 AND IMPLICATIONS FOR THE FORMATION OF CH+ [J].