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  Cold electron reactions producing the energetic isomer of hydrogen cyanide in interstellar clouds

Mendes, M. B., Buhr, H., Berg, M. H., Froese, M., Grieser, M., Heber, O., et al. (2012). Cold electron reactions producing the energetic isomer of hydrogen cyanide in interstellar clouds. The Astrophysical Journal Letters, 746: L8, pp. 1-5. doi:10.1088/2041-8205/746/1/L8.

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http://iopscience.iop.org/2041-8205/746/1/L8/ (Publisher version)
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 Creators:
Mendes, Mario B.1, Author           
Buhr, Hendrik1, 2, Author           
Berg, Max H.1, Author           
Froese, Michael1, Author           
Grieser, Manfred1, Author           
Heber, Oded2, Author
Jordon-Thaden, Brandon1, Author           
Krantz, Claude1, Author           
Novotný, Oldrich1, 3, Author           
Novotny, Steffen1, Author           
Orlov, Dmitry A.1, Author           
Petrignani, Annemieke1, Author           
Rappaport, Michael L.2, Author
Repnow, Roland1, Author           
Schwalm, Dirk1, Author           
Shornikov, Andrey1, Author           
Stützel, Julia1, Author           
Zajfman, Daniel2, Author
Wolf, Andreas1, Author           
Affiliations:
1Division Prof. Dr. Klaus Blaum, MPI for Nuclear Physics, Max Planck Society, ou_904548              
2Weizmann Institute of Science, P.O. Box 26, 76100 Rehovot, Israel, ou_persistent22              
3Columbia Astrophysics Laboratory, MC 5247, 550 West 120th Street, New York, New York 10027, USA, ou_persistent22              

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 Abstract: Using event-by-event fragment momentum spectroscopy in a storage-ring merged-beams experiment, we find laboratory evidence that in the dissociative recombination (DR) of HCNH+ with cold electrons the energetic isomer HNC is produced with a high yield, similar to that of HCN. With a newly implemented mass-sensitive fragment imaging detector, we analyze the kinetic energy release of the triatomic fragments DCN/DNC from the DR reaction of the isotopologue DCND+with cold (near 10 K) electrons. The results show that the internal energy of these fragments is extremely high, far exceeding the isomerization barrier between DNC and DCN. From this laboratory characterization of the DR reaction we conclude that also the triatomic fragment HCN/HNC from the DR of HCNH+ will carry a large amount of ro-vibrational excitation and show that this implies an isomeric production ratio in a narrow range near unity.

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Language(s): eng - English
 Dates: 2012-02-10
 Publication Status: Issued
 Pages: 5
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1088/2041-8205/746/1/L8
 Degree: -

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Title: The Astrophysical Journal Letters
  Other : Astrophys. J. Lett.
Source Genre: Journal
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Publ. Info: Chicago, IL : University of Chicago Press for the American Astronomical Society
Pages: - Volume / Issue: 746 Sequence Number: L8 Start / End Page: 1 - 5 Identifier: ISSN: 0004-637X
CoNE: https://pure.mpg.de/cone/journals/resource/954922828215