The systemic velocity of beta Lyrae

Astronomy and Astrophysics – Astronomy

Scientific paper

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Eclipsing Binary Stars, Orbital Elements, Radial Velocity, Stellar Spectra, Variable Stars, Circular Orbits, Line Spectra, Orbit Calculation, Tables (Data)

Scientific paper

Radial velocities of beta Lyr are determined from spectrograms obtained at Victoria, Canada, from 1966 to 1974. Individual stellar velocities and phases are calculated, and the radial velocities are found to be well satisfied by an assumed circular orbit with a systemic velocity of about -17.8 km/sec and a velocity of 184.0 km/sec for the primary component, provided that account is taken of the changing period in calculating the phases and the velocity measurements are made only from the Si II lines. Previous reports indicating variations in the value of the systemic velocity are discussed, and it is shown that the reported variations may be due to the use of unreliable spectral lines for velocity measurement, small systematic differences between spectrographs, and possible occasional distortion of the velocity curve.

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