| Literature DB >> 9506936 |
B J McCall1, T R Geballe, K H Hinkle, T Oka.
Abstract
The molecular ion H3+ is considered the cornerstone of interstellar chemistry because it initiates the reactions responsible for the production of many larger molecules. Recently discovered in dense molecular clouds, H3+ has now been observed in the diffuse interstellar medium toward Cygnus OB2 No. 12. Analysis of H3+ chemistry suggests that the high H3+ column density (3.8 x 10(14) per square centimeter) is due not to a high H3+ concentration but to a long absorption path. This and other work demonstrate the ubiquity of H3+ and its potential as a probe of the physical and chemical conditions in the interstellar medium.Entities:
Mesh:
Substances:
Year: 1998 PMID: 9506936 DOI: 10.1126/science.279.5358.1910
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728