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A long hard-X-ray look at the dual active galactic nuclei of M51 with NuSTAR

Brightman, M.; Baloković, M.; Koss, M.; Alexander, D.M.; Annuar, A.; Earnshaw, H.; Gandhi, P.; Harrison, F.A.; Hornschemeier, A.E.; Lehmer, B.; Powell, M.C.; Ptak, A.; Rangelov, B.; Roberts, T.P.; Stern, D.; Walton, D.J.; Zezas, A.

A long hard-X-ray look at the dual active galactic nuclei of M51 with NuSTAR Thumbnail


M. Brightman

M. Baloković

M. Koss

D.M. Alexander

A. Annuar

H. Earnshaw

P. Gandhi

F.A. Harrison

A.E. Hornschemeier

B. Lehmer

M.C. Powell

A. Ptak

B. Rangelov

D. Stern

D.J. Walton

A. Zezas


We present a broadband X-ray spectral analysis of the M51 system, including the dual active galactic nuclei (AGN) and several off-nuclear point sources. Using a deep observation by NuSTAR, new high-resolution coverage of M51b by Chandra, and the latest X-ray torus models, we measure the intrinsic X-ray luminosities of the AGN in these galaxies. The AGN of M51a is found to be Compton thick, and both AGN have very low accretion rates (λEdd<10−4). The latter is surprising considering that the galaxies of M51 are in the process of merging, which is generally predicted to enhance nuclear activity. We find that the covering factor of the obscuring material in M51a is 0.26±0.03, consistent with the local AGN obscured fraction at LX∼1040 erg s−1. The substantial obscuring column does not support theories that the torus, presumed responsible for the obscuration, disappears at these low accretion luminosities. However, the obscuration may have resulted from the gas infall driven by the merger rather than the accretion process. We report on several extra-nuclear sources with LX>1039 erg s−1 and find that a spectral turnover is present below 10 keV in most such sources, in line with recent results on ultraluminous X-ray sources.


Brightman, M., Baloković, M., Koss, M., Alexander, D., Annuar, A., Earnshaw, H., …Zezas, A. (2018). A long hard-X-ray look at the dual active galactic nuclei of M51 with NuSTAR. Astrophysical Journal, 867(2), Article 110.

Journal Article Type Article
Acceptance Date Sep 12, 2018
Online Publication Date Nov 5, 2018
Publication Date Nov 5, 2018
Deposit Date Oct 10, 2018
Publicly Available Date Nov 19, 2018
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 867
Issue 2
Article Number 110
Related Public URLs


Published Journal Article (2.7 Mb)

Copyright Statement
© 2018. The American Astronomical Society. All rights reserved.

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