Multi-wavelength study of the Be/X-ray binary MXB 0656-072

TL;DR

This study provides a comprehensive multi-wavelength analysis of the Be/X-ray binary MXB 0656-072, revealing its orbital period, mass ejection events, and X-ray spectral characteristics during outbursts, enhancing understanding of its accretion dynamics.

Contribution

First detection of the 101.2-day orbital period and detailed correlation between optical and X-ray behaviors in MXB 0656-072.

Findings

Orbital period of 101.2 days identified.

Mass ejection event indicated by anti-correlation in optical data.

X-ray spectra fit well with a cut-off power law and show a cyclotron feature.

Abstract

We present and analyze the optical photometric and spectroscopic data of the Be/X-ray binary MXB 0656-072 from 2006 to 2009. A 101.2-day orbital period is found, for the first time, from the present public X-ray data(Swift/BAT and RXTE/ASM). The anti-correlation between the H$\alpha$ emission and the $UBV$ brightness of MXB 0656$-$072 during our 2007 observations indicates that a mass ejection event took place in the system. After the mass ejection, a low-density region might develop around the Oe star. With the outward motion of the circumstellar disk, the outer part of the disk interacted with the neutron star around its periastron passage and a series of the X-ray outbursts were triggered between MJD 54350 and MJD 54850. The PCA--HEXTE spectra during the 2007-2008 X-ray outbursts could be well fitted by a cut-off power law with low energy absorption, together with an iron line around 6.4 keV, and a broad cyclotron resonance feature around 30 keV. The same variability of the soft and hard X-ray colors in 2.3-21 keV indicated that there were no overall changes in the spectral shape during the X-ray outbursts, which might be only connected with the changes of the mass-accretion rate onto the neutron star.