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26 April 2024
 
  » arxiv » 1007.0662

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Astronomical identification of CN-, the smallest observed molecular anion
M. Agundez ; J. Cernicharo ; M. Guelin ; C. Kahane ; E. Roueff ; J. Klos ; F. J. Aoiz ; F. Lique ; N. Marcelino ; J. R. Goicoechea ; M. Gonzalez Garcia ; C. A. Gottlieb ; M. C. McCarthy ; P. Thaddeus ;
Date 5 Jul 2010
AbstractWe present the first astronomical detection of a diatomic negative ion, the cyanide anion CN-, as well as quantum mechanical calculations of the excitation of this anion through collisions with para-H2. CN- is identified through the observation of the J = 2-1 and J = 3-2 rotational transitions in the C-star envelope IRC +10216 with the IRAM 30-m telescope. The U-shaped line profiles indicate that CN-, like the large anion C6H-, is formed in the outer regions of the envelope. Chemical and excitation model calculations suggest that this species forms from the reaction of large carbon anions with N atoms, rather than from the radiative attachment of an electron to CN, as is the case for large molecular anions. The unexpectedly large abundance derived for CN-, 0.25 % relative to CN, makes likely its detection in other astronomical sources. A parallel search for the small anion C2H- remains so far unconclusive, despite the previous tentative identification of the J = 1-0 rotational transition. The abundance of C2H- in IRC +10216 is found to be vanishingly small, < 0.0014 % relative to C2H.
Source arXiv, 1007.0662
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