Four-colour photometry of the double-mode Cepheid EW Scuti

Details Four-colour photometry of the double-mode Cepheid EW Scuti Four-colour photometry of the double-mode Cepheid EW Scuti

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.249..563f&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 249, April 1, 1991, p. 563-566. FNRS-supported research

Astronomy and Astrophysics

Astronomy

7

Cepheid Variables, Light Curve, Stellar Magnitude, Stellar Spectrophotometry, Ubv Spectra, Photographic Plates, Scutum Constellation, Variable Stars

Scientific paper

uvby observations of the double-mode Cepheid EW Scuti are presented, and
the first photoelectric light curves related to the two periods P0 =
5.8232 + or - 0.0002 d and P1 = 4.0673 + or - 0.0002 d are provided. A
frequency analysis of the data yields an adequate solution for the light
variation of EW Sct.

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