X-ray Gyrations of Eta Carinae, or, Is Presence of Evidence Evidence of Presence?
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We review the properties of the variable X-ray emission from the extremely massive star Eta Carinae concentrating on the last X-ray minimum, and briefly consider the possible role of a binary companion star on the observational properties of the system.
submitted to the proceedings of "Massive Stars In Interacting Binaries", Aug 16-20 2004, Quebec
submitted to the proceedings of "Massive Stars In Interacting Binaries", Aug 16-20 2004, Quebec