The Emission Spectrum of T Tau in 1971-1979

Physics

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Scientific paper

We present the results of our long-time homogeneous low-resolution spectroscopy of T Tau, the prototype T Tauri star. We show that the star's spectral activity was different at different times of the observations and possibly was cyclic, with a many-year cycle. Variable emission activity in spectral lines at different brightness ranges was revealed. During the star's brightest state, equivalent widths of hydrogen emission lines show variations up to the factor of 5. The observed properties of the emission spectrum can be explained by the disk-accretion theory.

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