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arXiv · 0801.0834

Determination of tidal distortion in the eclipsing binary system V621 Cen by means of deviations from the third Kepler law

Lorenzo Iorio
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Abstract

In this paper we determine the tidal distortion parameter k_m of the secondary partner (mass loser) of the semi-detached eclipsing binary system V621 Cen by comparing the phenomenologically determined orbital period P_b=3.683549(11) d to the Keplerian one P^Kep computed with the values of the relevant system's parameters determined independently of the third Kepler law itself. Our result is k_m = -1.5 +/- 0.6. Using the periastron precession, as traditionally done with other eclipsing binaries in eccentric orbits, would have not been possible because of the circularity of the V621 Cen path.

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Lorenzo Iorio. 2008-01-06. Determination of tidal distortion in the eclipsing binary system V621 Cen by means of deviations from the third Kepler law. https://doi.org/10.1016/j.newast.2008.01.004

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