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We present a consistent model atmosphere analysis and evolutionary tracks for the very nearby G‐type star 82 Eri that was most recently announced by Pepe et al. to harbour two or three super‐Earth companions with orbital periods of 18, 40 and 90 d. As a bright and high‐velocity object, 82 Eri was already realized by Jan Hendrik Oort in his 1926 treatise to be of ‘probably different origin’ and we...
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