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: http://www.stsci.edu/stsci/meetings/planets/abs/prog21.html
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We have observed 51 Peg alone and during the transit of the planet in front of the star on Aug. 18, 19, 27, 29, Sept. 3 and 4 1996 with CSHELL at IRTF and CGS4 at UKIRT. Our aim is to look for absorption lines from the material evaporated around the planet while occulting the star that would enable us to infer information on the nature of the atmosphere around the planet. The data reduction is currently under way and we will present preliminary results.
Last update: 10/22/96 11:00:29