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The interstellar synthesis of ammonia
The reaction H3+ + N → NH2+ +H has been measured in the laboratory at room temperature for the first time. It is sufficiently fast (k = 4.5 × 10−10 cm3 s−1) to provide a larger source of NH3 in dense interstellar clouds at 10 K than the more widely accepted source N+ + H2. At 50 K, both ion-molecule...
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Published in: | Monthly notices of the Royal Astronomical Society 1997-10, Vol.290 (4), p.636-638 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that cite this one |
Online Access: | Request full text |
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Summary: | The reaction H3+ + N → NH2+ +H has been measured in the laboratory at room temperature for the first time. It is sufficiently fast (k = 4.5 × 10−10 cm3 s−1) to provide a larger source of NH3 in dense interstellar clouds at 10 K than the more widely accepted source N+ + H2. At 50 K, both ion-molecule mechanisms (H3+ + N and N+ + H2) may provide roughly equivalent sources of NH3. |
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ISSN: | 0035-8711 1365-2966 |
DOI: | 10.1093/mnras/290.4.636 |