000002819 001__ 2819
000002819 005__ 20160701171711.0
000002819 0247_ $$2DOI$$a10.1017/S1743921311011574
000002819 037__ $$aASTROimport-976
000002819 100__ $$aMartayan, C.
000002819 245__ $$aHigh-angular resolution observations of the Pistol star
000002819 260__ $$c2011
000002819 520__ $$aFirst results of near-IR adaptive optics (AO)-assisted imaging, interferometry, and spectroscopy of this Luminous Blue Variable (LBV) are presented. They suggest that the Pistol Star is at least double. If the association is physical, it would reinforce questions concerning the importance of multiplicity for the formation and evolution of extremely massive stars. 
000002819 700__ $$a Blomme, R.
000002819 700__ $$a Le Bouquin, J.-B.
000002819 700__ $$a Merand, A.
000002819 700__ $$a Montagnier, G.
000002819 700__ $$a Selman, F.
000002819 700__ $$a Girard, J.
000002819 700__ $$a Fox, A.
000002819 700__ $$a Baade, D.
000002819 700__ $$a Frémat, Y.
000002819 700__ $$a Lobel, A.
000002819 700__ $$a Martins, F.
000002819 700__ $$a Patru, F.
000002819 700__ $$a Rivinius, T.
000002819 700__ $$a Sana, H.
000002819 700__ $$a Štefl, S.
000002819 700__ $$a Zorec, J.
000002819 700__ $$a Semaan, T.
000002819 773__ $$c616-617$$pActive OB Stars: Structure, Evolution, Mass Loss, and Critical Limits$$v272$$y2011
000002819 85642 $$ahttp://esoads.eso.org/abs/2011IAUS..272..616M
000002819 905__ $$apublished in
000002819 980__ $$aNONREF