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Cited article:

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Long-term Evolution in Ionization of Ejecta Illuminated by Eta Carinae

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The Long-term Spectral Changes of Eta Carinae: Are they Caused by a Dissipating Occulter as Indicated by cmfgen Models?

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The orbital kinematics of η Carinae over three periastra with a possible detection of the elusive secondary’s motion

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Did a close tidal encounter cause the Great Dimming of Betelgeuse?

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Eta Carinae: An Evolving View of the Central Binary, Its Interacting Winds and Its Foreground Ejecta

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Changes in the Na D1 Absorption Components of η Carinae Provide Clues on the Location of the Dissipating Central Occulter

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The Altered State of η Carinae: HST’s Photometric Record 1998–2021*

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Wind collision and accretion simulations of the massive binary system HD 166734

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Simulating the response of the secondary star of Eta Carinae to mass accretion at periastron passage

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Eta Carinae’s Declining Outflow Seen in the UV, 2002–2015*

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The 2014 X-Ray Minimum of η Carinae as Seen by Swift

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VLTI-AMBER velocity-resolved aperture-synthesis imaging ofηCarinae with a spectral resolution of 12 000

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He II λ4686 EMISSION FROM THE MASSIVE BINARY SYSTEM IN η CAR: CONSTRAINTS TO THE ORBITAL ELEMENTS AND THE NATURE OF THE PERIODIC MINIMA* † ‡ §

M. Teodoro, A. Damineli, B. Heathcote, N. D. Richardson, A. F. J. Moffat, L. St-Jean, C. Russell, T. R. Gull, T. I. Madura, K. R. Pollard, F. Walter, A. Coimbra, R. Prates, E. Fernández-Lajús, R. C. Gamen, G. Hickel, W. Henrique, F. Navarete, T. Andrade, F. Jablonski, P. Luckas, M. Locke, J. Powles, T. Bohlsen, R. Chini, et al.
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