The determination of the rotational periods of rapidly oscillating AP stars from their mean light variations. III - HR 3831 (HD 83368)

Statistics – Computation

Scientific paper

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A Stars, Light Curve, Magnetic Stars, Stellar Oscillations, Stellar Rotation, Variable Stars, Computational Astrophysics, Low Frequencies, Pulsars

Scientific paper

We have obtained new B mean light observations of HR 3831 in 1985 and new BVRI mean light observations in 1987. A frequency analysis of the new observations along with previous observations leads to a revised rotational ephemeris for HR 3831 of
HJD (extremum)=2440001.06 ±2.851962 E ±0.02 ±0.000014
where the extremum is maximum brightness in u, v and B and minimum brightness in y, V, R and I. The rotational frequency for HR 3831 is now known to an accuracy of 20 pHz and is frot=4.05829±0.00002μHz.

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