UBV photometry of the Beta Cephei type variable stars. V - 16 (EN) Lacertae

Details UBV photometry of the Beta Cephei type variable stars. V - 16 (EN) Lacertae UBV photometry of the Beta Cephei type variable stars. V - 16 (EN) Lacertae

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aca....43...13j&link_type=abstract

Acta Astronomica (ISSN 0001-5237), vol. 43, no. 1, p. 13-26.

Astronomy and Astrophysics

Astronomy

19

Cepheid Variables, Eclipsing Binary Stars, Stellar Spectrophotometry, Ubv Spectra, Least Squares Method, Stellar Magnitude, Stellar Oscillations

Scientific paper

Extensive B, BV, and UBV photoelectric observations of the eclipsing system 16 Lacertae, which has a Beta Cephei primary, obtained in 1964 and 1965 are presented and analyzed. The primary's light variation consists of nine sinusoidal terms, six of them discovered in the present analysis. Amplitudes, periods, color amplitude to visual amplitude ratios, and spherical harmonic orders of the underlying oscillations are obtained.

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