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J.A. Eisner, B.F. Lane (Caltech)
We have conducted observations of several Herbig Ae/Be stars with the Palomar Testbed Interferometer. These represent the longest baseline near-IR interferometric observations of this class of objects to date. We find that most of the observed sources are resolved, and we determine the angular size scale of the circumstellar emission under the assumptions of uniform disk, inclined disk, and Gaussian models.
The author(s) of this abstract have provided an email address for comments about the abstract: jae@astro.caltech.edu
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Bulletin of the American Astronomical Society, 34, #4
© 2002. The American Astronomical Soceity.