Investigating the origin of the faint non-thermal emission of the Arches cluster using the 2015–2016NuSTARandXMM–NewtonX-ray observations-Reference-Cited by-同舟云学术

Investigating the origin of the faint non-thermal emission of the Arches cluster using the 2015–2016NuSTARandXMM–NewtonX-ray observations

Published:2019-01-16 Issue:2 Volume:484 Page:1627-1636
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Kuznetsova Ekaterina¹,Krivonos Roman¹^ORCID,Clavel Maïca²,Lutovinov Alexander¹³,Chernyshov Dmitry⁴,Hong JaeSub⁵,Mori Kaya⁶,Ponti Gabriele⁷,Tomsick John⁸,Zhang Shuo⁹^ORCID

Affiliation:

1. Space Research Institute of the Russian Academy of Sciences, Profsoyuznaya 84/32, 117997 Moscow, Russia

2. Univ. Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France

3. Higher School of Economics, Myasnitskaya 20, 101000 Moscow, Russia

4. I.E. Tamm Theoretical Physics Division of P.N. Lebedev Institute of Physics, Leninskii pr. 53, 119991 Moscow, Russia

5. Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA

6. Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA

7. Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, Garching, D-85748, Germany

8. Space Sciences Laboratory, University of California, 7 Gauss Way, Berkeley, CA 94720-7450, USA

9. MIT Kavli Institute, 77 Massachusetts Ave, Cambridge, MA 02139 USA

Funder

National Aeronautics and Space Administration

Russian Foundation for Basic Research

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/484/2/1627/27583319/stz119.pdf

Reference41 articles.

1. Discovery of X-ray flaring activity in the Arches cluster

2. Fe Kαline emission from the Arches cluster region – evidence for ongoing particle bombardment?

3. Time Variability of Equivalent Width of 6.4 keV Line from the Arches Complex: Reflected X-Rays or Charged Particles?

4. Glimpses of the past activity of Sgr A★ inferred from X-ray echoes in Sgr C

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