X-ray Gyrations of Eta Carinae, or, Is Presence of Evidence Evidence of Presence?

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dc.creatorCorcoran, M. F.
dc.creatorHamaguchi, K.
dc.creatorGull, T.
dc.creatorDamineli, A.
dc.creatorDavidson, K.
dc.date2004-11-08
dc.date.accessioned2026-07-07T02:15:43Z
dc.date.available2026-07-07T02:15:43Z
dc.descriptionWe 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.
dc.descriptionsubmitted to the proceedings of "Massive Stars In Interacting Binaries", Aug 16-20 2004, Quebec
dc.identifierhttps://arxiv.org/abs/astro-ph/0411213
dc.identifierhttp://arxiv.org/abs/astro-ph/0411213
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8511
dc.subjectAstrophysics
dc.titleX-ray Gyrations of Eta Carinae, or, Is Presence of Evidence Evidence of Presence?
dc.typetext

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