Fourier Decomposition Parameters for the Rr-Lyrae Stars U-Caeli and V-Caeli

Details Fourier Decomposition Parameters for the Rr-Lyrae Stars U-Caeli and V-Caeli Fourier Decomposition Parameters for the Rr-Lyrae Stars U-Caeli and V-Caeli

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cto..conf..272h&link_type=abstract

Cepheids: Theory and Observations, Proceedings of IAU Colloquium No. 82, held 29 May - 1 June, 1984 in Toronto, Canada. Edited

Computer Science

2

Scientific paper

UBVRI light curves are obtained for the two halo RR Lyrae variables U Caeli with period 0.420 days and V Caeli with period 0.571 days. It is shown that their light curve characteristics are very similar to those of field RR Lyrae stars. Fourier decompositions are studied for all five magnitudes and the resulting amplitude ratios and phase differences are discussed.

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