Summary
Between 1997.0 and 2004.3, a series of observations were accomplished with the Hubble Space Telescope Imaging Spectrograph (HST/STIS) and from 2002.9 to 2005.3 with the Very Large Telescope/Ultraviolet Echelle Spectrograph (VLT/UVES). Coordinated observations were also done with RXTE, CHANDRA, FUSE and several ground-based telescopes. Much new information has been obtained about this Luminous Blue Variable (LBV) which appears to be a binary star system with at least one component being in very late stages of CNO-burning. These observations are summarized with intent on suggesting future observations with the VLT and VLT(I) especially during the upcoming apastron (2006.25) and periastron (2009.0).
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Gull, T.R. (2007). The Ejecta of Eta Carinae: What we have Learned from Space Telescope Imaging Spectrograph and the Ultraviolet Echelle Spectrograph. In: Richichi, A., Delplancke, F., Paresce, F., Chelli, A. (eds) The Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation. Eso Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-74256-2_16
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