Literature DB >> 9506936

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

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.

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Year:  1998        PMID: 9506936     DOI: 10.1126/science.279.5358.1910

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  3 in total

1.  Chemistry, astronomy and physics of H3+.

Authors:  Takeshi Oka
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2012-11-13       Impact factor: 4.226

2.  Interstellar H(3)(+).

Authors:  Takeshi Oka
Journal:  Proc Natl Acad Sci U S A       Date:  2006-08-07       Impact factor: 11.205

3.  Dissociative recombination of H3+: 10 years in retrospect.

Authors:  Mats Larsson
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2012-11-13       Impact factor: 4.226

  3 in total

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