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W.A. Traub (Harvard-Smithsonian CfA), R.S. Millan-Gabet (CfA and U. Mass.), M.R. Garcia (CfA)
We spatially resolved the symbiotic star CI Cam, about 6 months after its April 1998 outburst, using the IOTA stellar interferometer. We measured the diameter of the dust shell in the H and K infrared bands over a range of position angles. We will discuss the relationship between these results and other ongoing observations of CI Cam.
The author(s) of this abstract have provided an email address for comments about the abstract: traub@cfa.harvard.edu