Swift-BAT hard X-ray sky monitoring unveils the orbital period of the HMXB IGR J18219-1347

TL;DR

This study analyzes INTEGRAL BAT survey data to identify a 72.46-day orbital period of the HMXB IGR J18219-1347, revealing its variability and suggesting it hosts a Be star based on X-ray emission patterns.

Contribution

First detection of the orbital period of IGR J18219-1347 using BAT survey data, providing insights into its binary system characteristics.

Findings

Detected a 72.46-day orbital period with high significance.

Observed strong variability and emission only during a small orbital phase.

Spectral analysis indicates a flat absorbed power law with a cutoff at ~11 keV.

Abstract

IGR J18219-1347 is a hard X-ray source discovered by INTEGRAL in 2010. We have analyzed the X-ray emission of this source exploiting the BAT survey data up to March 2012 and the XRT data that include also an observing campaign performed in early 2012. The source is detected at a significance level of ~14 standard deviations in the 88-month BAT survey data, and shows a strong variability along the survey monitoring, going from high intensity to quiescent states. A timing analysis on the BAT data revealed an intensity modulation with a period of 72.46 days. The significance of this modulation is about 7 standard deviations in Gaussian statistics. We interpret it as the orbital period of the binary system. The light curve folded at P_0 shows a sharp peak covering ~30% of the period, superimposed to a flat level roughly consistent with zero. In the soft X-rays the source is detected only in 5 out of 12 XRT observations, with the highest recorded count rate corresponding to a phase close to the BAT folded light curve peak. The long orbital period and the evidence that the source emits only during a small fraction of the orbit suggests that the IGR J18219-1347 binary system hosts a Be star. The broad band XRT+BAT spectrum is well modeled with a flat absorbed power law with a high energy exponential cutoff at ~11 keV.