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M.A. Shure, W.G. Bagnuolo, H.A. McAlister, J. Sturmann, L. Sturmann, T.A. ten Brummelaar (CHARA-Georgia State University), S.T. Ridgway (KPNO/NOAO/CHARA), N.H. Turner (MWI/CHARA)
We review the technical options available for near-infrared beam combination from the six 1-meter telescopes of the CHARA Interferometer on Mt Wilson, as well as the current status of the fringe imaging system.
MAS and LS acknowledge the support of NSF grant AST-9731183.
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The author(s) of this abstract have provided an email address for comments about the abstract: shure@chara.gsu.edu