On the machine computation of the orbits of eclipsing binaries

Details On the machine computation of the orbits of eclipsing binaries On the machine computation of the orbits of eclipsing binaries

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981rmxaa...6...99p&link_type=abstract

(International Astronomical Union, Reunion Regional Latinoamericana de Astronomia, 2nd, Merida, Venezuela, Jan. 19-23, 1981) Rev

Astronomy and Astrophysics

Astronomy

4

Computer Techniques, Eclipsing Binary Stars, Light Curve, Orbit Calculation, Astronomical Photometry, Error Analysis, Minima, Orbital Elements, Radiant Flux Density

Scientific paper

A discussion is presented concerning the most desirable practices that can be adopted in the use of computers to solve the light curves of eclipsing binaries. Great care must be exercised in evaluating meaningful parameter uncertainties, and it is sugested that investigators have two completely independent sets of observations, obtained at different times and by different observers, available.

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