Source:http://linkedlifedata.com/resource/pubmed/id/12673244
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rdf:type | |
lifeskim:mentions | |
pubmed:issue |
6931
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pubmed:dateCreated |
2003-4-3
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pubmed:abstractText |
The H3+ molecular ion plays a fundamental role in interstellar chemistry, as it initiates a network of chemical reactions that produce many molecules. In dense interstellar clouds, the H3+ abundance is understood using a simple chemical model, from which observations of H3+ yield valuable estimates of cloud path length, density and temperature. But observations of diffuse clouds have suggested that H3+ is considerably more abundant than expected from the chemical models. Models of diffuse clouds have, however, been hampered by the uncertain values of three key parameters: the rate of H3+ destruction by electrons (e-), the electron fraction, and the cosmic-ray ionization rate. Here we report a direct experimental measurement of the H3+ destruction rate under nearly interstellar conditions. We also report the observation of H3+ in a diffuse cloud (towards Persei) where the electron fraction is already known. From these, we find that the cosmic-ray ionization rate along this line of sight is 40 times faster than previously assumed. If such a high cosmic-ray flux is ubiquitous in diffuse clouds, the discrepancy between chemical models and the previous observations of H3+ can be resolved.
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pubmed:language |
eng
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pubmed:journal | |
pubmed:status |
PubMed-not-MEDLINE
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pubmed:month |
Apr
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pubmed:issn |
0028-0836
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pubmed:author |
pubmed-author:Al-KhaliliAA,
pubmed-author:DjuricNN,
pubmed-author:DunnG HGH,
pubmed-author:EhlerdingAA,
pubmed-author:GeballeT RTR,
pubmed-author:HellbergFF,
pubmed-author:HuneycuttA JAJ,
pubmed-author:KalhoriSS,
pubmed-author:LarssonMM,
pubmed-author:McCallB JBJ,
pubmed-author:NealHH,
pubmed-author:NovotnyOO,
pubmed-author:OsterdahlFF,
pubmed-author:SaykallyR JRJ,
pubmed-author:SemaniakJJ,
pubmed-author:ThomasRR
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pubmed:issnType |
Print
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pubmed:day |
3
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pubmed:volume |
422
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pubmed:owner |
NLM
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pubmed:authorsComplete |
Y
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pubmed:pagination |
500-2
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pubmed:dateRevised |
2003-11-4
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pubmed:year |
2003
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pubmed:articleTitle |
An enhanced cosmic-ray flux towards zeta Persei inferred from a laboratory study of the H3+-e- recombination rate.
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pubmed:affiliation |
Department of Chemistry, Department of Astronomy, University of California at Berkeley, Berkeley, California 94720, USA. bjmccall@astro.berkeley.edu
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pubmed:publicationType |
Journal Article
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