The Principal Frequency in the Light Variation of HD101065

Details The Principal Frequency in the Light Variation of HD101065 The Principal Frequency in the Light Variation of HD101065

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.196...61k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 196, P. 61, 1981

Astronomy and Astrophysics

Astronomy

9

Scientific paper

Further observations of the light variability of HD 101065 have been obtained in 1980 which remove the cycle count ambiguity in the principal frequency. Assuming the principal frequency is stable over the two years for which observations are available, its value can now be given as f= 4.942316 ± 0.000023 which is equivalent to a period of 12.14006 ± 0.00006 min. The ephemeris is Tmax(B) = HJD 2443400.00090(1) + 0.00843060(4).n. All of the photometric data obtained from 1978 to 1980 are made available with this paper.

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