Statistics – Computation
Scientific paper
Apr 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.231.1039k&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 231, April 15, 1988, p. 1039-1046. Research supported b
Statistics
Computation
9
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.
Kurtz Don W.
Marang Freddy
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