# Spectral analysis of the dipping LMXB system XB 1916-053

## TL;DR

This study analyzes Suzaku observations of the dipping LMXB XB 1916-053, revealing details about its spectral state, ionized absorption features, and the nature of seed photons involved in Comptonization, with implications for accretion physics.

## Contribution

It provides the first detection of extit{K} extsubscript{eta} absorption lines of highly ionized iron in XB 1916-053 and clarifies the origin of seed photons in the system.

## Key findings

- The source remains in a soft spectral state across observations.
- Detection of extit{K} extsubscript{eta} lines of Fe XXV and Fe XXVI.
- Identification of an extit{O} extsubscript{VIII} absorption edge.

## Abstract

Context: XB 1916-053 is a low mass X-ray binary system (LMXB) hosting a neutron star (NS) and showing periodic dips. The spectrum of the persistent emission was modeled with a blackbody component having a temperature between 1.31 and 1.67 keV and with a Comptonization component with an electron temperature of 9.4 keV and a photon index $\Gamma$ between 2.5 and 2.9. The presence of absorption features associated with highly ionized elements suggested the presence of partially ionized plasma in the system. Aims: In this work we performed a study of the spectrum of XB 1916-053, which aims to shed light on the nature of the seed photons that contribute to the Comptonization component. Methods: We analyzed three Suzaku observations of XB 1916-053: the first was performed in November 2006 and the others were carried out in October 2014. We extracted the persistent spectra from each observation and combined the spectra of the most recent observations, obtaining a single spectrum with a higher statistic. We also extracted and combined the spectra of the dips observed during the same observations. Results: On the basis of the available data statistics, we infer that the scenario in which the corona Comptonizes photons emitted both by the innermost region of the accretion disk and the NS surface is not statistically relevant with respect to the case in which only photons emitted by the NS surface are Comptonized. We find that the source is in a soft spectral state in all the analyzed observations. We detect the K$\alpha$ absorption lines of \ion{Fe}{xxv} and \ion{Fe}{xxvi}, which have already been reported in literature, and for the first time the K$\beta$ absorption lines of the same ions. We also detect an edge at 0.876 keV, which is consistent with a \ion{O}{viii} K absorption edge. (Abridged)