A light echo from the warm outflow in the ULIRG F01004-2237 following a major flare in its optical continuum emission

TL;DR

This study observes a light echo in the ULIRG F01004-2237, revealing how a past optical flare affected its outflow regions, and suggests the flare may be due to a tidal disruption event in an active galaxy.

Contribution

First detection of a light echo from a warm outflow in a ULIRG following a major optical flare, providing insights into the outflow structure and flare origin.

Findings

Broad emission line wings associated with the flare have declined in flux.

Forbidden lines' blue wings have increased, indicating outflow response.

First detection of the [FeVII](6087) line in this galaxy.

Abstract

Emission-line variability studies have the potential to provide key information about the structures of the near-nuclear outflow regions of AGN. Here we present a VLT/Xshooter spectrum of the nucleus of the ULIRG F01004-2237 that was taken in August 2018, about 8 yr after a major flare in its integrated optical emission. Compared with our WHT/ISIS spectrum from September 2015, the broad, red wings of the emission lines most closely associated with the flaring event, including HeII(4686), NIII(4100,4640) and HeI(5876), have substantially declined in flux. In contrast, the broad, blue wings that dominate the [OIII], [NeIII], [NeV] and [OI] forbidden lines have increased in flux by a factor 1.4 - 4.4 (depending on the line). Moreover, the [FeVII](6087) line is detected in the new spectrum for the first time. We interpret these results in terms of a light echo from the outflowing warm gas: the direct emission from the flaring event is continuing to fade, but due to light travel time effects we are only now observing the impact of the flare on the emission from the extended outflow region. Unless the outflow is confined to a small range of angles close to our line of sight, these observations imply that the outflow must be relatively compact (r<50 pc). In terms of the nature of the flare event, we speculate that the properties of the F01004-2237 flare may be the result of a tidal disruption event (TDE) occurring in an object with pre-existing AGN activity.