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Detection of a Noble Gas Molecular Ion, 36ArH+, in the Crab Nebula

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Science  13 Dec 2013:
Vol. 342, Issue 6164, pp. 1343-1345
DOI: 10.1126/science.1243582

Article Information

vol. 342 no. 6164 1343-1345

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History: 
  • Received for publication July 22, 2013
  • Accepted for publication November 5, 2013
  • .

Author Information

  1. M. J. Barlow1,*,
  2. B. M. Swinyard1,2,
  3. P. J. Owen1,
  4. J. Cernicharo3,
  5. H. L. Gomez4,
  6. R. J. Ivison5,
  7. O. Krause6,
  8. T. L. Lim2,
  9. M. Matsuura1,
  10. S. Miller1,
  11. G. Olofsson7,
  12. E. T. Polehampton2,8
  1. 1Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK.
  2. 2Space Science and Technology Department, Rutherford Appleton Laboratory, Didcot OX11 0QX, UK.
  3. 3Laboratory of Molecular Astrophysics, Department of Astrophysics, Centro de Astrobiologia, Instituto Nacional de Tecnicas Aeroespaciales–Consejo Superior de Investigaciones Cientificas, Ctra de Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain.
  4. 4School of Physics and Astronomy, Cardiff University, The Parade, Cardiff CF24 3AA, UK.
  5. 5UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK.
  6. 6Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany.
  7. 7Department of Astronomy, Stockholm University, AlbaNova University Center, Roslagstulsbacken 21, 10691 Stockholm, Sweden.
  8. 8Institute for Space Imaging Science, Department of Physics and Astronomy, University of Lethbridge, Lethbridge, Alberta T1K 3M4, Canada.
  1. *Corresponding author. E-mail: mjb{at}star.ucl.ac.uk

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