Radial velocity measurements of u¹ Bootis

dc.contributor.authorNiehaus, Russell Josephen_US
dc.date.accessioned2024-08-15T16:35:27Z
dc.date.available2024-08-15T16:35:27Z
dc.date.copyright1970en_US
dc.date.issued1970
dc.degree.departmentDepartment of Physics
dc.degree.departmentDepartment of Physics and Astronomy
dc.degree.levelMaster of Science M.Sc.en
dc.description.abstractRadial velocity measurements of spectrograms of μ¹ Bootis taken at the Dominion Astrophysical Observatory in Victoria show no evidence for variability in the radial velocity of the star, with either a short or a long period. This conclusion was reached after statistical tests for variability were performed on the data. A comparison of radial velocity measurements from normal contrast, Kodak IIa0, plates and high contrast, Kodak III0, plates reveals no detectable gain in accuracy from the use of high contrast. Measurements of radial velocities of μ¹ Bootis made with the oscilloscope machine are internally more consistent than those made with visual measuring machines. The mean radial velocity of μ¹ Bootis, taken over 83 measure­ments each of unit weight, is -13 .0 km/sec, with a standard error of about 2 km/sec. This large standard error is chiefly the result of errors in the effective wavelengths adopted for the star.en
dc.format.extent172 pages
dc.identifier.urihttps://hdl.handle.net/1828/19158
dc.rightsAvailable to the World Wide Weben_US
dc.titleRadial velocity measurements of u¹ Bootisen_US
dc.typeThesisen_US

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