Analysis and Comparison of CCD and RVS Radial Velocities for Three delta Scuti Variable Stars

Details Analysis and Comparison of CCD and RVS Radial Velocities for Three delta Scuti Variable Stars Analysis and Comparison of CCD and RVS Radial Velocities for Three delta Scuti Variable Stars

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...20111705m&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #117.05; Bulletin of the American Astronomical Society, Vol. 34, p.1296

Astronomy and Astrophysics

Astrophysics

Scientific paper

Observations have been obtained of AI Canum Venaticorum, V966 Herculis, and GW Draconis using both the Radial Velocity Scanner (RVS) and the Site CCD system on the 1.2-meter telescope of the Dominion Astrophysical Observatory. Using these three δ Scuti variables we compare the radial velocities determined by the two systems to examine the advantages and disadvantages of each type of observation for the production of high precision radial velocity curves. Preliminary results will be presented.

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