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The evolutionary status of eta Car based on historical and modern optical and infrared photometry
Authors:A M van Genderen  M de Groot  P S The
Institution:(1) Leiden Observatory, Leiden, Netherlands;(2) Armagh Observatory, Armagh, UK;(3) Astronomical Institute, Amsterdam
Abstract:We present a photometric study of the luminous early-type star eegr Car. The star's secular brightness increase is due largely to the expansion of the Homunculus. eegr Car is a LBV with a possible B0.5V companion. The combined effect of Balmer-line emission, and of warm and cold dust radiation explains the star's other light variations.
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