CaltechAUTHORS
  A Caltech Library Service

IC 751: a new changing-look AGN discovered by NuSTAR

Ricci, C. and Bauer, F. E. and Arevalo, P. and Boggs, S. and Brandt, W. N. and Christensen, F. E. and Craig, W. W. and Gandhi, P. and Hailey, C. J. and Harrison, F. A. and Koss, M. and Markwardt, C. B. and Stern, D. and Treister, E. and Zhang, W. W. (2016) IC 751: a new changing-look AGN discovered by NuSTAR. Astrophysical Journal, 820 (1). Art. No. 5. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20160317-141351548

[img] PDF - Published Version
See Usage Policy.

857Kb
[img] PDF - Submitted Version
See Usage Policy.

716Kb

Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20160317-141351548

Abstract

We present results of five Nuclear Spectroscopic Telescope Array (NuSTAR) observations of the type 2 active galactic nucleus (AGN) in IC 751, three of which were performed simultaneously with XMM-Newton or Swift/X-Ray Telescope. We find that the nuclear X-ray source underwent a clear transition from a Compton-thick (N_H ≃ 2 x 10^(24)cm^(-2)) to a Compton-thin (N_H ≃ 4 x 10^(23) cm^(-2)) state on timescales of ≾ 3 months, which makes IC 751 the first changing look AGN discovered by NuSTAR. Changes of the line of sight column density at the ~2σ level are also found on a timescale of ~48 hr (ΔN_H ~ 10^(23cm^(-2)). From the lack of spectral variability on timescales of ~100 ks, we infer that the varying absorber is located beyond the emission-weighted average radius of the broad-line region (BLR), and could therefore be related either to the external part of the BLR or a clumpy molecular torus. By adopting a physical torus X-ray spectral model, we are able to disentangle the column density of the non-varying absorber (N_H ~ 3.8 x 10^(23)cm^(-2)) from that of the varying clouds [N_H ~ (1-150) x 10^(22 cm^(-2)], and to constrain that of the material responsible for the reprocessed X-ray radiation (N_H ~ 6 x 10^(24) cm^(-2)). We find evidence of significant intrinsic X-ray variability, with the flux varying by a factor of five on timescales of a few months in the 2–10 and 10–50 keV band.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.3847/0004-637X/820/1/5DOIArticle
http://iopscience.iop.org/article/10.3847/0004-637X/820/1/5PublisherArticle
http://arxiv.org/abs/1602.00702arXivDiscussion Paper
ORCID:
AuthorORCID
Ricci, C.0000-0001-5231-2645
Bauer, F. E.0000-0002-8686-8737
Boggs, S.0000-0001-9567-4224
Brandt, W. N.0000-0002-0167-2453
Gandhi, P.0000-0003-3105-2615
Harrison, F. A.0000-0003-2992-8024
Koss, M.0000-0002-7998-9581
Stern, D.0000-0003-2686-9241
Additional Information:© 2016 American Astronomical Society. Received 2015 November 28; accepted 2016 January 20; published 2016 March 10. We thank the anonymous referee for comments that helped us to improve the quality of our manuscript. CR acknowledges Marko Stalevski and Sebastien Guillot for fruitful discussions, and Chin-Shin Chang for her comments on the manuscript. This research has made use of the NuSTAR Data Analysis Software (NuSTARDAS) jointly developed by the ASI Science Data Center (ASDC, Italy) and the California Institute of Technology (Caltech, USA). We acknowledge financial support from the CONICYT-Chile grants "EMBIGGEN" Anillo ACT1101 (CR, ET, FEB, PA), FONDECYT 1141218 (CR, FEB), FONDECYT 1140304 (PA), Basal-CATA PFB-06/2007 (CR, ET, FEB), NuSTAR subcontract 44A-1092750 (WNB), the Swiss National Science Foundation and Ambizione fellowship grant PZ00P2 154799/1 (MK), and the Ministry of Economy, Development, and Tourism's Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS (FEB). This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, of data obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), provided by NASA's Goddard Space Flight Center, and of the SIMBAD Astronomical Database which is operated by the Centre de Données astronomiques de Strasbourg. Facilities: NuSTAR - The NuSTAR (Nuclear Spectroscopic Telescope Array) mission, Swift - Swift Gamma-Ray Burst Mission, XMM-Newton - .
Group:NuSTAR, Infrared Processing and Analysis Center (IPAC), Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
Comisión Nacional de Investigación Científica y Tecnológica (CONICyT)Anillo ACT1101
Fondo Nacional de Desarrollo Científico y Tecnológico (FONDECYT)1141218
Fondo Nacional de Desarrollo Científico y Tecnológico (FONDECYT)1140304
Basal-CATAPFB-06/2007
NuSTAR44A-1092750
Swiss National Science Foundation (SNSF)PZ00P2 154799/1
Iniciativa Científica Milenio del Ministerio de Economía, Fomento y TurismoIC120009
Subject Keywords:galaxies: active; galaxies: individual:IC 751; galaxies: Seyfert; X-rays: galaxies
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2016-04
Record Number:CaltechAUTHORS:20160317-141351548
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20160317-141351548
Official Citation:C. Ricci et al 2016 ApJ 820 5
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:65450
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:17 Mar 2016 22:46
Last Modified:21 Mar 2019 18:54

Repository Staff Only: item control page