Optimal set of photometric elements of the eclipsing variable TZ Bootis

Details Optimal set of photometric elements of the eclipsing variable TZ Bootis Optimal set of photometric elements of the eclipsing variable TZ Bootis

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.134..153a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 134, no. 1, June 1987, p. 153-159.

Astronomy and Astrophysics

Astrophysics

3

Astronomical Photometry, Eclipsing Binary Stars, Light Curve, Electrophotometry, Fourier Analysis

Scientific paper

The eclipsing system of W UMa-type TZ Bootis has been examined on the basis of six light curves analyzed by the means of the Fourier techniques. An optimal resulting set of geometric elements for the system is obtained from both minima, through there magnitudes variations during the periods 1967, 1969, 1974, 1976, 1978, and 1980. The intrinsic variability of the system has been discussed in the light of the behaviour of the light curves.

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