NASA NTRS · 20120009344
X-Ray Variability and the Secondary Star
Abstract
We discuss the history of X-ray observations of the 11 Car system, concentrating on the periodic variability discovered in the 1990s. We discuss the interpretation of these variations, concentrating on a model of the system as a "collidingwind" binary. This interpretation allows the physical and orbital parameters of eta Car and its companion star to be constrained.
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Corcoran, M. F., Ishibashi, K.. 2012-01-01. X-Ray Variability and the Secondary Star. https://ntrs.nasa.gov/citations/20120009344
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