UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

Changing-look Event in NGC 3516: Continuum or Obscuration Variability?

Mehdipour, Missagh; Kriss, Gerard A; Brenneman, Laura W; Costantini, Elisa; Kaastra, Jelle S; Branduardi-Raymont, Graziella; Di Gesu, Laura; ... Mao, Junjie; + view all (2022) Changing-look Event in NGC 3516: Continuum or Obscuration Variability? The Astrophysical Journal , 925 (1) , Article 84. 10.3847/1538-4357/ac42ca. Green open access

[thumbnail of Mehdipour+_NGC3516_2021.pdf]
Preview
Text
Mehdipour+_NGC3516_2021.pdf - Accepted Version

Download (975kB) | Preview

Abstract

The Seyfert-1 galaxy NGC 3516 has undergone major spectral changes in recent years. In 2017 we obtained Chandra, NuSTAR, and Swift observations during its new low-flux state. Using these observations, we model the spectral energy distribution (SED) and the intrinsic X-ray absorption, and compare the results with those from historical observations taken in 2006. We thereby investigate the effects of the changing-look phenomenon on the accretion-powered radiation and the ionized outflows. Compared to its normal high-flux state in 2006, the intrinsic bolometric luminosity of NGC 3516 was lower by a factor of 4–8 during 2017. Our SED modeling shows a significant decline in the luminosity of all the continuum components from the accretion disk and the X-ray source. As a consequence, the reprocessed X-ray emission lines have also become fainter. The Swift monitoring of NGC 3516 shows remarkable X-ray spectral variability on short (weeks) and long (years) timescales. We investigate whether this variability is driven by obscuration or the intrinsic continuum. We find that the new low-flux spectrum of NGC 3516, and its variability, do not require any new or variable obscuration, and instead can be explained by changes in the ionizing SED that result in the lowering of the ionization of the warm-absorber outflows. This in turn induces enhanced X-ray absorption by the warm-absorber outflows, mimicking the presence of new obscuring gas. Using the response of the ionized regions to the SED changes, we place constraints on their densities and locations.

Type: Article
Title: Changing-look Event in NGC 3516: Continuum or Obscuration Variability?
Open access status: An open access version is available from UCL Discovery
DOI: 10.3847/1538-4357/ac42ca
Publisher version: https://doi.org/10.3847/1538-4357/ac42ca
Language: English
Additional information: Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
UCL classification: UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL
URI: https://discovery.ucl.ac.uk/id/eprint/10142663
Downloads since deposit
124Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item