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

Boller, Th.; Keil, R.; Hasinger, G.; Costantini, E.; Fujimoto, R.; Anabuki, N.; Lehmann, I.; Gallo, L.

doi:10.1051/0004-6361:20031217

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

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

/persons/resource/persons23324

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

/persons/resource/persons16194

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

/persons/resource/persons22927

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

/persons/resource/persons23425

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

/persons/resource/persons23075

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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