ИСТИНА

Up to now all well-established magnetars are isolated objects. Still, there are some candidates to NSs with high magnetic field in accreting X-ray binary systems, mostly with massive donors. In this talk I review observational data on these objects and discuss how their existence fits models of formation and evolution of NS magnetic field. Some specific combination of parameters allows existence of NSs with magnetar-sclae fields in HMXBs. Most probably, these compact objects are on the Hall attractor stage.