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1 Introduction: Multiplicity of brown dwarfs
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2 Our targets: Cha H
1 to 12
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3 HST observation and data reduction
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4 Ground-based imaging with VLT and NTT
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5 Real companions or background objects?
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6 The promising candidate near Cha H
5
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7 Is Cha H
2 a close binary?
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8 Discussion
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References
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