# Space Telescope and Optical Reverberation Mapping Project. X. Understanding the Absorption-Line Holiday in NGC 5548

## TL;DR

This study investigates the unusual 'holiday' in emission-line variability in NGC 5548, revealing that changes in soft X-ray ionization caused by an obscurer explain the decoupling from UV-optical continuum variations.

## Contribution

The paper introduces a novel model linking absorption line variability and soft X-ray continuum changes to explain the emission-line holiday in NGC 5548.

## Key findings

- Absorption line variability correlates with the emission-line holiday.
- Soft X-ray continuum changes influence helium ionization in the broad-line region.
- A new cycle reproduces the observed absorption line behavior during the holiday.

## Abstract

The flux variations in the emission lines in active galactic nuclei (AGNs) are driven by variations in the ionizing continuum flux --which are usually reflected in the observable UV-optical continuum. The "Reverberation mapping" technique measures the delay between line and continuum variations to determine the size of the line emitting region, this is the basis for measurements of the central black hole mass in AGNs. The Space Telescope and Optical Reverberation Mapping Project (AGN STORM) on NGC 5548 in 2014 is the most intensive multi-wavelength AGN monitoring campaign ever. For most of the campaign, the emission-line variations followed changes in the continuum with a time lag, as expected. However, the lines varied independently of the observed UV-optical continuum during a 60 -- 70 day "holiday." To understand this remarkable phenomenon, we study the intrinsic absorption lines present in NGC 5548. We identify a novel cycle that reproduces the absorption line variability and thus identify the physics that allows the holiday to occur. In our model, variations in this obscurer's line-of-sight covering factor modify the soft X-ray continuum. This leads to changes in the ionization of helium gas in the broad-line region. Ionizing radiation produced by recombining helium then affects the ionization of other species as observed during the AGN STORM holiday. It is likely that any other model which selectively changes the soft X-ray part of the continuum during the holiday can also explain the anomalous emission line behavior observed.

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Source: https://tomesphere.com/paper/1812.11578