Historical Perspective On the Study of Epsilon Aurigae

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Scientific paper

Epsilon Aurigae has been known since 1821 as an eclipsing binary with a 27 year period, but has defied interpretation for nearly 2 centuries. The high luminosity F star is eclipsed by an invisible companion, now recognized as a debris-like disk. I will briefly review prior ideas proposed by Struve, Eggleton and Huang and others, to set the stage for the remarkable revelations made possible during the current 2009-2011 eclipse.

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