Light curves and solutions for ST Centauri

Details Light curves and solutions for ST Centauri Light curves and solutions for ST Centauri

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86.1546m&link_type=abstract

Astronomical Journal, vol. 86, Oct. 1981, p. 1547-1552. Research supported by the Natural Sciences and Engineering Research Cou

Astronomy and Astrophysics

Astronomy

7

Astrometry, Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Asymmetry, Classifications, Ubv Spectra

Scientific paper

The reported investigation is an extension of a study conducted by O'Connell (1951). UBV photoelectric observations and classification dispersion spectroscopy studies were conducted of several eclipsing binaries during a period of 40 days. A description is given of photometric results and qualitative aspects of the spectroscopy of ST Cen. Extinction and transformation coefficients are listed in a table. The differential (V-C) magnitudes and color indices are also presented, and the V, B, and U differential observations are shown in a graph. A light curve analysis is discussed. In addition to the asymmetry in the light curve maxima, noticeable scatter is found among the data points in each maximum.

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