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  Investigating the origin of the faint non-thermal emission of the Arches cluster using the 2015–2016 NuSTAR and XMM–Newton X-ray observations

Kuznetsova, E., Krivonos, R., Clavel, M., Lutovinov, A., Chernyshov, D., Hong, J., et al. (2019). Investigating the origin of the faint non-thermal emission of the Arches cluster using the 2015–2016 NuSTAR and XMM–Newton X-ray observations. Monthly Notices of the Royal Astronomical Society, 484(2), 1627-1636. doi:10.1093/mnras/stz119.

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Kuznetsova, Ekaterina, Author
Krivonos, Roman, Author
Clavel, Maïca, Author
Lutovinov, Alexander, Author
Chernyshov, Dmitry, Author
Hong, JaeSub, Author
Mori, Kaya, Author
Ponti, Gabriele1, Author           
Tomsick, John, Author
Zhang, Shuo, Author
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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 Dates: 2019-01-16
 Publication Status: Published online
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 Rev. Type: Peer
 Identifiers: DOI: 10.1093/mnras/stz119
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Title: Monthly Notices of the Royal Astronomical Society
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Source Genre: Journal
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Publ. Info: OXFORD : OXFORD UNIV PRESS
Pages: - Volume / Issue: 484 (2) Sequence Number: - Start / End Page: 1627 - 1636 Identifier: ISSN: 0035-8711
CoNE: https://pure.mpg.de/cone/journals/resource/1000000000021470