IGR J19294+1816: a new Be-X ray binary revealed through infrared spectroscopy

TL;DR

This study identifies IGR J19294+1816 as a Be X-ray binary through infrared spectroscopy, revealing its nature, distance, and luminosity, and marking the first infrared spectrum of this source.

Contribution

First infrared spectrum of IGR J19294+1816, confirming it as a Be X-ray binary and accurately determining its distance and luminosity.

Findings

Classified the donor as a B1Ve star

Estimated the distance as 11 ± 1 kpc

Confirmed the source as a transient Be X-ray binary

Abstract

The aim of this work is to characterize the counterpart to the INTEGRAL High Mass X-ray Binary candidate IGR J19294+1816 so as to establish its true nature. We obtained H band spectra of the selected counterpart acquired with the NICS instrument mounted on the Telescopio Nazionale Galileo (TNG) 3.5-m telescope which represents the first infrared spectrum ever taken of this source. We complement the spectral analysis with infrared photometry from UKIDSS, 2MASS, WISE and NEOWISE databases. We classify the mass donor as a Be star. Subsequently, we compute its distance by properly taking into account the contamination produced by the circumstellar envelope. The findings indicate that IGR J19294+1816 is a transient source with a B1Ve donor at a distance of $d = 11 \pm 1$ kpc, and luminosities of the order of $10^{36-37}$ erg s$^{-1}$, displaying the typical behaviour of a Be X-ray binary.