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FU Orionis Resolved by Infrared Long-Baseline Interferometry at a 2 AU Scale

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F. Malbet1, J.-P. Berger1, M. M. Colavita2, C. D. Koresko3, C. Beichman2,4, A. F. Boden2, S. R. Kulkarni3, B. F. Lane3, D. W. Mobley2, X. P. Pan3, M. Shao2, G. T. Van Belle2 and J. K. Wallace2

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