Am. Vangenderen et al., THE EVOLUTIONARY STATUS OF ETA-CAR BASED ON HISTORICAL AND MODERN OPTICAL AND INFRARED PHOTOMETRY, Space science reviews, 66(1-4), 1993, pp. 219-223
We present a photometric study of the luminous early-type star eta Car
. The star's secular brightness increase is due largely to the expansi
on of the Homunculus. Eta Car is a LBV with possible B0.5V companion.
The combined effect of Balmer-line emission, and of warm and col dust
radiation explains the star's other light variations.