The Hercules-Lyra association revisited - New age estimation and multiplicity study

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Fig. 4

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The HH Leo (=HD 96064) system from 2002 (Calar Alto Ω-Cass with ALFA, inset left), through 2005 (inset middle), to 2008 (inset right and main image, both VLT/NaCo). Orbital motion of the BC component can clearly be seen. For further explanations see text.

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