Demonstration Science: the Chromosphere of Alpha Tau

Physics

Scientific paper

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Hst Proposal Id #3023

Scientific paper

The C II intercombination lines (UV 0.01) near 2325 A will be used to estimate the turbulent velocity and electron density in the chromosphere of the K giant Alpha Tau. High S/N Mg II profiles will be acquired to search for discrete absorption features superposed on the emission lines. LSA and SSA observations using echelle B and G270M are made to allow experiments with deconvolution of LSA and medium resolution data.

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