Turner, TJ, Reeves, JN, Braito, V, Lobban, AP, Kraemer, S and Miller, L (2018) A rapid occultation event in NGC 3227. Monthly Notices of the Royal Astronomical Society, 481 (2). 2470 -2478. ISSN 1365-2966

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NGC 3227 exhibits rapid flux and spectral variability in the X-ray band. To understand this behaviour, we conducted a coordinated observing campaign using 320 ks of XMM–Newton exposures together with 160 ks of overlapping NuSTAR observations, spanning a month. Here, we present a rapid variability event that occurs toward the end of the campaign. The spectral hardening event is accompanied by a change in the depth of an unresolved transition array (UTA), whose time-dependent behaviour is resolved using the RGS data. This UTA fingerprint allows us to identify this as a transit event, where a clump of gas having NH∼5×1022atomscm−2⁠, log ξ ∼ 2 occults ∼60 per cent of the continuum photons over the course of approximately a day. This occulting gas is likely associated with clouds in the inner broad-line region. An additional zone of gas with lower column and higher ionization, matches the outflow velocity of the variable zone, and may represent transmission through the cloud limb.

Item Type: Article
Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Uncontrolled Keywords: galaxies, active, individual, NGC 3227, Seyfert, X-rays
Subjects: Q Science > QB Astronomy > QB460 Astrophysics
Q Science > QB Astronomy > QB799 Stars
Divisions: Faculty of Natural Sciences > School of Chemical and Physical Sciences
Depositing User: Symplectic
Date Deposited: 06 Dec 2018 10:32
Last Modified: 09 Mar 2021 09:35
URI: https://eprints.keele.ac.uk/id/eprint/5549

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