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  Dissociative Recombination Measurements of NH+ Using an Ion Storage Ring

Novotný, O., Becker, A., Buhr, H., Domesle, C., Geppert, W., Grieser, M., et al. (2014). Dissociative Recombination Measurements of NH+ Using an Ion Storage Ring. The Astrophysical Journal, 792(2): 132. doi:10.1088/0004-637X/792/2/132.

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Novotný, O.1, Author
Becker, Arno2, Author           
Buhr , H.1, Author
Domesle, C.2, Author           
Geppert, W.3, Author
Grieser, M.2, Author           
Krantz, C.2, Author           
Kreckel, H.2, Author           
Repnow, R.2, Author           
Schwalm, D2, 4, Author           
Spruck, Kaija2, Author           
Stützel, J1, 2, Author           
Yang , B.1, 5, Author
Wolf, A.2, Author           
Savin, D. W.1, Author
Affiliations:
1 Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA , ou_persistent22              
2Division Prof. Dr. Klaus Blaum, MPI for Nuclear Physics, Max Planck Society, ou_904548              
3Department of Physics, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden , ou_persistent22              
4 Institut für Atom- und Molekülphysik, Justus-Liebig-Universität Giessen, D-35392 Giessen, Germany , ou_persistent22              
5 Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China , ou_persistent22              

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 MPINP: Quantendynamik - Abteilung Blaum
 Abstract: We have investigated dissociative recombination (DR) of NH+ with electrons using a merged beams configuration at the TSR heavy-ion storage ring located at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany. We present our measured absolute merged-beams recombination rate coefficient for collision energies from 0 to 12 eV. From these data, we have extracted a cross section, which we have transformed to a plasma rate coefficient for the collisional plasma temperature range from Tpl = 10 to 18,000 K. We show that the NH+ DR rate coefficient data in current astrochemical models are underestimated by up to a factor of approximately nine. Our new data will result in predicted NH+ abundances lower than those calculated by present models. This is in agreement with the sensitivity limits of all observations attempting to detect NH+ in interstellar clouds.

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 Dates: 2014-08-26
 Publication Status: Published online
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1088/0004-637X/792/2/132
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Title: The Astrophysical Journal
Source Genre: Journal
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Publ. Info: Chicago, IL : University of Chicago Press for the American Astronomical Society
Pages: - Volume / Issue: 792 (2) Sequence Number: 132 Start / End Page: - Identifier: ISSN: 0004-637X
CoNE: https://pure.mpg.de/cone/journals/resource/954922828215_3