Should we see iron features in the AGN model of the X-ray background?

  • R. Gilli, G. Brunetti, G. Setti, A. Comastri
  • Astronomische Nachrichten, January 1998, Wiley
  • DOI: 10.1002/asna.2123190129

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http://dx.doi.org/10.1002/asna.2123190129

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