XMM-Newton and Swift observations of XTE J1743-363

TL;DR

This study presents XMM-Newton and Swift observations of XTE J1743-363, confirming its classification as a Symbiotic X-ray Binary with wind accretion, high absorption, and variable X-ray flares, enhancing understanding of such systems.

Contribution

First dedicated soft X-ray monitoring of XTE J1743-363 confirming its nature as a Symbiotic X-ray Binary with detailed variability analysis.

Findings

Confirmed association with M8 III giant

Detected high absorption (~6x10^22 cm^-2)

Observed a faint ~4 ks flare

Abstract

XTEJ1743-363 is a poorly known hard X-ray transient, that displays short and intense flares similar to those observed from Supergiant Fast X-ray Transients. The probable optical counterpart shows spectral properties similar to those of an M8 III giant, thus suggesting that XTEJ1743-363 belongs to the class of the Symbiotic X-ray Binaries. In this paper we report on the first dedicated monitoring campaign of the source in the soft X-ray range with XMM-Newton and Swift/XRT. T hese observations confirmed the association of XTEJ1743-363 with the previously suggested M8 III giant and the classification of the source as a member of the Symbiotic X-ray binaries. In the soft X-ray domain, XTEJ1743-363 displays a high absorption (~6x10^22 cm^-2 ) and variability on time scales of hundreds to few thousand seconds, typical of wind accreting systems. A relatively faint flare (peak X-ray flux 3x10^-11 erg/cm^2/s) lasting ~4 ks is recorded during the XMM-Newton observation and interpreted in terms of the wind accretion scenario.