Variability of the symbiotic X-ray binary GX 1+4

Enhanced activity near periastron passage

¹ Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00716 Warsaw, Poland
e-mail: krystian.ilkiewicz@gmail.com
² Kleinkaroo Observatory, Calitzdorp, Western Cape, South Africa

Received: 7 November 2016
Accepted: 22 February 2017

Abstract

Context. GX 1+4 belongs to a rare class of X-ray binaries with red giant donors, symbiotic X-ray binaries. It has a history of complicated variability on multiple timescales in the optical light and X-rays. The nature of this variability remains poorly understood.

Aims. We aim to study variability of GX 1+4 on long timescale in X-ray and optical bands.

Methods. We took X-ray observations from the INTEGRAL Soft Gamma-Ray Imager and RXTE All Sky Monitor. Optical observations were made with the INTEGRAL Optical Monitoring Camera.

Results. The variability of GX 1+4 both in optical light and hard X-ray emission (>17 keV) is dominated by ~50–70 d quasi-periodic changes. The amplitude of this variability is highest during the periastron passage, while during the potential neutron star eclipse the system is always at minimum. This confirms the 1161 d orbital period that has had been proposed for the system based on radial velocity curve. Neither the quasi-periodic variability or the orbital period are detected in soft X-ray emission (1.3–12.2 keV), where the binary shows no apparent periodicity.