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Investigating the Origin of the Absorption-line Variability in the Narrow-line Seyfert 1 Galaxy WPVS 007
Journal article   Open access   Peer reviewed

Investigating the Origin of the Absorption-line Variability in the Narrow-line Seyfert 1 Galaxy WPVS 007

Kaylie S. Green, Sarah C. Gallagher, Karen M. Leighly,  Hyunseop Choi, Dirk Grupe, Donald M. Terndrup, Gordon T. Richards and S. Komossa
The Astrophysical journal, v 953(2), 186
17 Aug 2023
url
https://doi.org/10.3847/1538-4357/ace2c4View
Published, Version of Record (VoR)CC BY V4.0 Open

Abstract

Active galactic nuclei Broad-absorption line quasar Quasars Spectroscopy
Broad absorption line quasars are actively accreting supermassive black holes that have strong outflows characterized by broad absorption lines in their rest-UV spectra. Variability in these absorption lines occurs over months to years depending on the source. WPVS 007, a low-redshift, low-luminosity narrow-line Seyfert 1 (NLS1) shows strong variability over shorter timescales, providing a unique opportunity to study the driving mechanism behind this variability that may mimic longer-scale variability in much more massive quasars. We present the first variability study using the spectral synthesis code SimBAL, which provides velocity-resolved changes in physical conditions of the gas using constraints from multiple absorption lines. Overall, we find WPVS 007 to have a highly ionized outflow with a large mass-loss rate and kinetic luminosity. We determine the primary cause of the absorption-line variability in WPVS 007 to be a change in covering fraction of the continuum by the outflow. This study is the first SimBAL analysis where multiple epochs of observation were fit simultaneously, demonstrating the ability of SimBAL to use the time domain as an additional constraint in spectral models.

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Astronomy & Astrophysics
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