Photometric observations and light curve analysis of ST Aquarii

Details Photometric observations and light curve analysis of ST Aquarii Photometric observations and light curve analysis of ST Aquarii

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.151...29a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 151, no. 1, Jan. 1989, p. 29-38.

Astronomy and Astrophysics

Astrophysics

4

Astronomical Photometry, Eclipsing Binary Stars, Light Curve, Ubv Spectra, Fourier Transformation, Hertzsprung-Russell Diagram, Telescopes, Variable Stars

Scientific paper

The system of ST Aquarii has been obsraved in B and V filters at Kottamia Observatory in Egypt. Two light curves have been obtained and new times of minima have been calculated. The light curves have been analyzed using the theory of Fourier transform of light changes in frequency-domain, and new geometrical and physical elements have been obtained.

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