000002769 001__ 2769
000002769 005__ 20160701171710.0
000002769 037__ $$aASTROimport-926
000002769 100__ $$aMartayan, C.
000002769 245__ $$aOn the Binarity of LBV Stars
000002769 260__ $$c2012
000002769 520__ $$aWe report on the binarity of luminous blue variable stars observed with a set of techniques and instruments.  Among them, observations at high angular resolution with the VLT-NACO, the VLTI-AMBER and with spectrographs such as the VLT-XSHOOTER allowed us to find several LBV stars as binaries or having a potential companion.  In particular the LBV Pistol Star clearly presents radial velocity variations and line profiles modifications (double peak appearance). In addition, the absorption component of the P Cygni lines varies as well with the time indicating a potential wind structure variability.  Our observations also show directly for the first time a companion to at least one of the observed LBVs (HD 168625).  This one seems to affect the environment of the system. This system is known to be surrounded by several rings similar to those of SN1987A, possibly indicating a future supernova occurrence for this Galactic object.  These results show that Eta Car is no longer unique. 
000002769 700__ $$a Lobel, A.
000002769 700__ $$a Baade, D.
000002769 700__ $$a Blomme, R.
000002769 700__ $$a Frémat, Y.
000002769 700__ $$a LeBouquin, J.-B.
000002769 700__ $$a Selman, F.
000002769 700__ $$a Girard, J.
000002769 700__ $$a Mérand, A.
000002769 700__ $$a Montagnier, G.
000002769 700__ $$a Patru, F.
000002769 700__ $$a Mawet, D.
000002769 700__ $$a Martins, F.
000002769 700__ $$a Rivinius, T.
000002769 700__ $$a Štefl, S.
000002769 700__ $$a Zorec, J.
000002769 700__ $$a Semaan, T.
000002769 700__ $$a Mehner, A.
000002769 700__ $$a Kervella, P.
000002769 700__ $$a Sana, H.
000002769 700__ $$a Schödel, R.
000002769 773__ $$c293$$pCircumstellar Dynamics at High Resolution$$v464$$y2012
000002769 85642 $$ahttp://esoads.eso.org/abs/2012ASPC..464..293M
000002769 905__ $$apublished in
000002769 980__ $$aNONREF