Detection of H3+ in the diffuse interstellar medium toward Cygnus OB2 No. 12

B. J. McCall, T. R. Geballe, K. H. Hinkle, T. Oka

Research output: Contribution to journalArticlepeer-review

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 languageEnglish (US)
Pages (from-to)1910-1913
Number of pages4
JournalScience
Volume279
Issue number5358
DOIs
StatePublished - Mar 20 1998
Externally publishedYes

ASJC Scopus subject areas

  • General

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