Revised elements of the eclipsing binary EO AUR

Details Revised elements of the eclipsing binary EO AUR Revised elements of the eclipsing binary EO AUR

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..70..461r&link_type=abstract

Astrophysics and Space Science, vol. 70, no. 2, July 1980, p. 461-465. Research supported by the Consiglio Nazionale delle Rice

Astronomy and Astrophysics

Astrophysics

3

Eclipsing Binary Stars, Light Curve, Orbital Elements, Stellar Mass, Stellar Models, Computer Techniques, Main Sequence Stars, Radii, Size Determination, Stellar Luminosity, Stellar Spectrophotometry

Scientific paper

Von Schneller's (1962) light curve of EO Aur was solved by means of
Wood's (1972) computer model. The solution confirms that EO Aur is a
detached system. Interestingly, EO Aur appears to be anomalous since the
primary component seems to be closer to the main sequence than the
secondary.

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