Radial Velocities of Stars in the Georgia State University  (GSU) Speckle Program
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Observations of binary stars through the Georgia State speckle                  interferometry program can produce accurate binary orbits in                    angular units.  Furenlid will make matching radial-velocity                     observations to deduce accurate orbits, distances, luminosities,                and masses of the binary stars.  The observations are to be made                at the Cananea Observatory, located in Mexico, south of Tucson,                 with a new and specially designed spectrograph.                                                                                                                 Some of the most basic information in astronomy, about distances                and masses of stars, is derived from observations of binary stars.              Furenlid will take spectra and measure accurate radial velocities               of binary stars whose positions relative to each other have                     already been observed with high accuracy, using a technique                     recently implemented by co-investigator McAlister.  The two sets                of data together will yield accurate basic stellar information not              obtainable by any other means.
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{'Code': '121500', 'Text': 'STELLAR ASTRONOMY & ASTROPHYSC'}
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