Toward Mapping the Detailed Density Structure of Classical Be Circumstellar Disks

Physics

Scientific paper

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Scientific paper

We present the preliminary results of near contemporaneous optical and infrared spectroscopic observations of selected classical Be stars. We find strong evidence of oppositely oriented V/R hydrogen line profiles in the optical versus infrared spectra of ζ Tau, and briefly discuss how sustained contemporaneous optical and infrared spectroscopic observations might enable us to trace the detailed density structure of classical Be circumstellar disks.

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