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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Detaylı Bibliyografya
Asıl Yazarlar: Daranlot, Julien, Hincelin, Ugo, Bergeat, Astrid, Costes, Michel, Loison, Jean-Christophe, Wakelam, Valentine, Hickson, Kevin M.
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: National Academy of Sciences 2012
Konular:
Physical Sciences
Online Erişim: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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