A multi-epoch spectroscopic study of the BAL quasar APM 08279+5255: I. C IV absorption variability

TL;DR

This study presents a 14-year spectroscopic monitoring of the BAL quasar APM 08279+5255, revealing stability in the broad absorption feature shape, a decline and sharp increase in equivalent width and R-band flux, and correlations suggesting ionization-driven variability.

Contribution

First long-term multi-epoch spectroscopic analysis of a BAL quasar linking absorption variability with optical flux changes.

Findings

Broad absorption feature shape remains stable over time.

Equivalent width declines then sharply increases in 2011.

Correlation between absorption variability and R-band flux.

Abstract

Broad Absorption Lines indicate gas outflows with velocities from thousands km/s to about 0.2 the speed of light, which may be present in all quasars and may play a major role in the evolution of the host galaxy. The variability of absorption patterns can provide informations on changes of the density and velocity distributions of the absorbing gas and its ionization status. We collected 23 photometrical and spectro-photometrical observations at the 1.82m Telescope of the Asiago Observatory since 2003, plus other 5 spectra from the literature. We analysed the evolution in time of the equivalent width of the broad absorption feature and two narrow absorption systems, the correlation among them and with the R band magnitude. We performed a structure function analysis of the equivalent width variations. We present an unprecedented monitoring of a broad absorption line quasar based on 28 epochs in 14 years. The shape of broad absorption feature shows a relative stability, while its equivalent width slowly declines until it sharply increases during 2011. In the same time the R magnitude stays almost constant until it sharply increases during 2011. The equivalent width of the narrow absorption redwards of the systemic redshift only shows a decline. The broad absorption behaviour suggests changes of the ionisation status as the main cause of variability. We show for the first time a correlation of this variability with the R band flux. The different behaviour of the narrow absorption system might be due to recombination time delay. The structure function of the absorption variability has a slope comparable with typical optical variability of quasars. This is consistent with variations of the 200 A ionising flux originating in the inner part of the accretion disk.