Spectroscopic orbital elements of Kappa-2 Bootis B
G. Á. Bakos
Abstract
G. Á. Bakos
Abstract
The orbital elements of the spectroscopic binary star Kappa-2 Boo (HR 5328) are derived on the basis of radial velocity measurements covering 70 yr. Attention is given to the phase distribution of velocities and residuals. The period of the system is determined to be 1790 days, and the semiamplitude of the velocity curve is found to be 7.2 km/sec.
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The orbital elements of the spectroscopic binary star Kappa-2 Boo (HR 5328) are derived on the basis of radial velocity measurements covering 70 yr. Attention is given to the phase distribution of velocities and residuals. The period of the system is determined to be 1790 days, and the semiamplitude of the velocity curve is found to be 7.2 km/sec.
Key concepts: Kappa, Physics, Orbital elements, Astrophysics, Radial velocity, Binary number, Star (game theory), Phase (matter)