X-ray Variability and the Secondary Star
作者： M. F. Corcoran , K. Ishibashi
DOI: 10.1007/978-1-4614-2275-4_9
关键词:
摘要: We discuss the history of X-ray observations η Car system, concentrating on periodic variability discovered in 1990s. interpretation these variations, a model system as “colliding-wind” binary. This allows physical and orbital parameters its companion star to be constrained.
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