On the binarity of LBV stars

We report on the binarity of luminous blue variable stars observed with a set of techniques and instruments.
Among them, observations at high angular resolution with the VLT-NACO, the VLTI-AMBER and with spectrographs such as 
the VLT-XSHOOTER allowed us to find several LBV stars as binaries or having potential companion.
In particular the LBV Pistol Star clearly presents radial velocity variations and line profiles modifications (double peaks 
appearance). In addition, the absorption component of the PCygni lines varies too with the time indicating a potential wind 
structure variability.
Our observations also show directly for the first time a companion to at least one of the observed LBVs (HD168625).
This one seems to affect the environment of the system. This system is known to be surrounded by several rings similar  to 
those of SN1987A, possibly indicating a future supernova occurrence for this Galactic object.
These results show that Eta Car is no longer unique and that it is possible to do similar studies on other LBV stars.