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

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.

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 Creators:
Boller, Th.1, Author              
Keil, R.1, Author              
Hasinger, G.1, Author              
Costantini, E.1, Author              
Fujimoto, R., Author
Anabuki, N., Author
Lehmann, I.1, Author              
Gallo, L.1, Author              
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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Language(s): eng - English
 Dates: 2003
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: eDoc: 62580
DOI: 10.1051/0004-6361:20031217
Other: 7631
 Degree: -

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Title: Astronomy & Astrophysics
  Alternative Title : Astron. Astrophys.
Source Genre: Journal
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Affiliations:
Publ. Info: -
Pages: - Volume / Issue: 411 Sequence Number: - Start / End Page: 63 - 70 Identifier: ISSN: 0004-6361