NuSTAR observations of four nearby X-ray faint AGNs: low luminosity or heavy obscuration?. Issue 1 (27th June 2020)

• Record Type: Journal Article
• Authors: 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, S; Masini, A; Nardini, E; Ricci, C; Stern, D; Zappacosta, L
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 497:Issue 1(2020)
• Page Start: 229
• Page End: 245
• Publication Date: 2020-06-27
• Subjects: galaxies: active -- X-rays: individual: ESO 121-G6 -- X-rays: individual: NGC 660 -- X-rays: individual: NGC 3486 -- X-rays: individual: NGC 5195; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/staa1820
• Languages: English
• ISSNs: 0035-8711

Abstract

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 L 2–10 keV, obs ≲ 10 39 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 ( N H ) 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 ( N H > 10 23 cm −2 ; L 2–10 keV, int ∼ 10 41 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 L 2–10 keV, int < 10 39 erg s −1, i.e. genuine LLAGN. Both of the heavily obscured AGNs have L bol > 10 41 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.