η Carinae: Testing a Binary Orbit Model with the Hubble Space Telescope/Space Telescope Imaging Spectrograph
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Humphreys | R. Humphreys | K. Ishibashi | T. Gull | K. Davidson | Smith | Ishibashi | Davidson | Gull | N. Smith
[1] R. Humphreys,et al. HST/FOS Spectroscopy of ETA Carinae: The Star Itself, and Ejecta Within 0.3 Arcsec , 1995 .
[2] Kazunori Ishibashi,et al. Recurrent X-Ray Emission Variations of η Carinae and the Binary Hypothesis , 1999 .
[3] K. Davidson. Is Eta Carinae a long-period binary? , 1997 .
[4] S. White. Radio evidence for non-isotropic outflows from hot stars , 1999 .
[5] P. Conti,et al. Eta Carinae: a long period binary? , 1997 .
[6] M. Feast,et al. Variability of η Carinae , 1994 .
[7] Louis Antonelli,et al. The 5.52 Year Cycle of Eta Carinae , 1996 .
[8] R. Humphreys,et al. HST/GHRS Observations of the Compact Slow Ejecta of Eta Carinae , 1997 .
[9] P. Cox,et al. Discovery of a massive equatorial torus in the η Carinae stellar system , 1999, Nature.
[10] K. Ishibashi,et al. The X-ray light curve of Eta Carinae , 1998 .
[11] R. Humphreys,et al. An Unusual Brightening Of Eta Carinae , 1999 .