Ubiquitous yet forgotten: broad absorptions in the optical spectra of low-mass X-ray binaries

TL;DR

This study reveals that broad absorption features are common in the optical spectra of low-mass X-ray binaries during outbursts, providing new insights into their accretion disc structures and behaviors.

Contribution

It is the first comprehensive population study of broad absorptions in low-mass X-ray binaries, analyzing their properties and origins across multiple systems.

Findings

Broad absorptions are ubiquitous in low-mass X-ray binaries during outbursts.

Their detection is independent of inclination or compact object type, but favors systems with periods < 11 hours.

Absorptions are strongest at shorter wavelengths and are present across all X-ray states.

Abstract

Optical outburst spectra of low-mass X-ray binaries enable studies of extreme accretion and ejection phenomena. While some of their spectroscopic features have been analysed in detail, the appearance of broad absorptions in the optical regime has been traditionally neglected. In this work, we introduce the first population study dedicated to these features with the aim to understand their fundamental properties and discuss them in the context of their origin. We complement the study with a spectroscopic database of six low-mass X-ray binaries during outburst, in order to assess their evolution. We find that broad absorptions are ubiquitous, with the majority of black hole low-mass X-ray binaries exhibiting them in spite of a typically scarce outburst coverage. Their detection does not depend on the orbital inclination or the compact object nature, but they seem favoured in systems with orbital periods shorter than < 11 h. They predominantly occur in the hydrogen Balmer series, being stronger at shorter wavelengths, and they are detected across all X-ray states. We find that the normalised depth of these broad absorptions is anti-correlated with the system luminosity, and that they show constant line ratios over the whole sample. Based on these properties, we favour a scenario where BAs arise from a stable, optically thick layer of the accretion disc, below the hotter chromosphere-like region producing the emission line components. Our study is consistent with the continuous presence of broad absorptions during the whole outburst, with their visibility being conditioned by the emission lines filling the broad absorption profile and veiling by the X-ray reprocessed continuum.