Detection of H 3 + in the Diffuse Interstellar Medium Toward Cygnus OB2 No. 12

Author:

McCall B. J.123,Geballe T. R.123,Hinkle K. H.123,Oka T.123

Affiliation:

1. B. J. McCall and T. Oka, Department of Astronomy and Astrophysics, Department of Chemistry, and the Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA.

2. T. R. Geballe, Joint Astronomy Centre, University Park, Hilo, HI 96720, USA.

3. K. H. Hinkle, National Optical Astronomy Observatories, Tucson, AZ 85726, USA.

Abstract

The molecular ion H 3 + 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, H 3 + has now been observed in the diffuse interstellar medium toward Cygnus OB2 No. 12. Analysis of H 3 + chemistry suggests that the high H 3 + column density (3.8 × 10 14 per square centimeter) is due not to a high H 3 + concentration but to a long absorption path. This and other work demonstrate the ubiquity of H 3 + and its potential as a probe of the physical and chemical conditions in the interstellar medium.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference46 articles.

1. Herbst E., Klemperer W., Astrophys. J. 185, 505 (1973);

2. Watson W. D., ibid. 183, L17 (1973);

3. ; ibid. 188 35 (1974).

4. Geballe T. R., Oka T., Nature 384, 334 (1996).

5. B. J. McCall T. R. Geballe K. H. Hinkle T. Oka in preparation.

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