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Elemental nitrogen partitioning in dense interstellar clouds
Many chemical models of dense interstellar clouds predict that the majority of gas-phase elemental nitrogen should be present as N(2), with an abundance approximately five orders of magnitude less than that of hydrogen. As a homonuclear diatomic molecule, N(2) is difficult to detect spectroscopicall...
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| Autors principals: | , , , , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
National Academy of Sciences
2012
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| Matèries: | |
| Accés en línia: | https://ncbi.nlm.nih.gov/pmc/articles/PMC3387123/ https://ncbi.nlm.nih.gov/pubmed/22689957 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1200017109 |
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