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 OBS No. 12. Analysis of H3+ chemistry suggests that the high H3+ column density (3.8 x 1014 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.
Original language | English (US) |
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Pages (from-to) | 1910-1913 |
Number of pages | 4 |
Journal | Science |
Volume | 279 |
Issue number | 5358 |
DOIs | |
State | Published - Mar 20 1998 |
Externally published | Yes |
ASJC Scopus subject areas
- General