Identification of High Mass X-ray Binaries selected from XMM-Newton observations of the LMC

Abstract

The Large Magellanic Cloud (LMC) currently hosts around 23 high mass X-ray binaries (HMXBs) of which most are Be/X-ray binaries. The LMC XMM-Newton survey provided follow-up observations of previously known X-ray sources that were likely HMXBs, as well as identifying new HMXB candidates. In total 19 candidate HMXBs were selected based on their X-ray hardness ratios. In this paper we present red and blue optical spectroscopy, obtained with SALT and the SAAO 1.9-m telescope, plus a timing analysis of the long term optical light curves from OGLE to confirm the nature of these candidates. We find that 9 of the candidates are new Be/X-ray Binaries, substantially increasing the LMC Be/X-ray binary population. Furthermore, we present the optical properties of these new systems, both individually and as a group of all the BeXBs identified by the XMM-Newton survey of the LMC.

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• eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds
• RX J0529.8-6556: a BeXRB pulsar with an evolving optical period and out of phase X-ray outbursts
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• Origin of young accreting neutron stars in high-mass X-ray binaries in supernova remnants
• Monitoring the X-ray Variability of Bright X-ray Sources in M33