Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. NuSTAR observations of four nearby X-ray faint AGNs: low luminosity or heavy obscuration?
 

NuSTAR observations of four nearby X-ray faint AGNs: low luminosity or heavy obscuration?

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2020
Author(s)
Annuar, A.
•
Alexander, D. M.
•
Gandhi, P.
•
Lansbury, G. B.
•
Asmus, D.
•
Baloković, M.
•
Ballantyne, D. R.
•
Bauer, F. E.
•
Boorman, P. G.
•
Brandt, W. N.
•
Brightman, M.
•
Chen, C. -T. J.
•
Del Moro, A.
•
Farrah, D.
•
Harrison, F. A.
•
Koss, M. J.
•
Lanz, L.
•
MARCHESI, STEFANO  
•
Masini, A.
•
NARDINI, EMANUELE  
•
Ricci, C.
•
Stern, D.
•
Zappacosta, L.  
DOI
10.1093/mnras/staa1820
Abstract
We present NuSTAR (Nuclear Spectroscopic Telescope Array) observations of four active galactic nuclei (AGNs) located within 15 Mpc. These AGNs, namely ESO 121-G6, NGC 660, NGC 3486, and NGC 5195, have observed X-ray luminosities of L2-10 keV,obs ≲ 1039 erg s-1, classifying them as low-luminosity AGN (LLAGN). We perform broad-band X-ray spectral analysis for the AGN by combining our NuSTAR data with Chandra or XMM-Newton observations to directly measure their column densities (NH) and infer their intrinsic power. We complement our X-ray data with archival and new high-angular resolution mid-infrared (mid-IR) data for all objects, except NGC 5195. Based on our X-ray spectral analysis, we found that both ESO 121-G6 and NGC 660 are heavily obscured (NH > 1023 cm-2; L2-10 keV,int ∼ 1041 erg s-1), and NGC 660 may be Compton thick. We also note that the X-ray flux and spectral slope for ESO 121-G6 have significantly changed over the last decade, indicating significant changes in the obscuration and potentially accretion rate. On the other hand, NGC 3486 and NGC 5195 appear to be unobscured and just mildly obscured, respectively, with L2-10 keV,int < 1039 erg s-1, i.e. genuine LLAGN. Both of the heavily obscured AGNs have Lbol > 1041 erg s-1 and λEdd ≳ 10-3, and are detected in high-angular resolution mid-IR imaging, indicating the presence of obscuring dust on nuclear scale. NGC 3486, however, is undetected in high-resolution mid-IR imaging, and the current data do not provide stringent constraints on the presence or absence of obscuring nuclear dust in the AGN.
Volume
497
Issue
1
Start page
229
Uri
http://hdl.handle.net/20.500.12386/31196
Url
https://academic.oup.com/mnras/article/497/1/229/5863952
Issn Identifier
0035-8711
Ads BibCode
2020MNRAS.497..229A
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

2006.13583.pdf

Description
preprint
Size

1.74 MB

Format

Adobe PDF

Checksum (MD5)

fdad2767427a30767b92cfcbd79e9dc1

Loading...
Thumbnail Image
Name

staa1820.pdf

Description
Pdf editoriale
Size

3.58 MB

Format

Adobe PDF

Checksum (MD5)

caeb809dd1e3c177612a1e7b5deaf174

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback