A photometric analysis of the supergiant close binary, V453 Scorpii

Details A photometric analysis of the supergiant close binary, V453 Scorpii A photometric analysis of the supergiant close binary, V453 Scorpii

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87..901w&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 87, Dec. 1975, p. 901-907.

Astronomy and Astrophysics

Astronomy

13

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Supergiant Stars, Ubv Spectra, Parameterization, Spectrum Analysis, Tables (Data)

Scientific paper

Yellow and blue photometry of V453 Sco shows the character of the light curve to be completely different from that accepted from photographic estimates. In the present data, there are conspicuous photometric complications, but it has been possible to solve the light curves by synthesis procedures. Absolute dimensions for the component stars have been derived, and an attempt at understanding the systemic evolution is presented.

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