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XMM-Newton observation of the ULIRG NGC 6240. The physical nature of the complex Fe K line emission

MPS-Authors
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Boller,  Th.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Keil,  R.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Hasinger,  G.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Costantini,  E.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Lehmann,  I.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Gallo,  L.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Boller, T., Keil, R., Hasinger, G., Costantini, E., Fujimoto, R., Anabuki, N., et al. (2003). XMM-Newton observation of the ULIRG NGC 6240. The physical nature of the complex Fe K line emission. Astronomy & Astrophysics, 411, 63-70. doi:10.1051/0004-6361:20031217.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-E821-E
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