Physics
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3023e&link_type=abstract
HST Proposal ID #3023
Physics
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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