The eclipsing binary EG Serpentis

Details The eclipsing binary EG Serpentis The eclipsing binary EG Serpentis

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aj....105.2291t&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 105, no. 6, p. 2291-2298.

Astronomy and Astrophysics

Astronomy

5

Eclipsing Binary Stars, Stellar Spectrophotometry, Light Curve, Stellar Magnitude, Stellar Orbits

Scientific paper

Stromgren b,y photometry of the detached A-type eclipsing binary EG Serpentis was obtained. Combined with the radial velocity curves in Popper, it was used to determine anew the system's parameters using the Wilson-Devinney code. The age of the system is derived from a comparison with the Bertelli et al. (1990) isochrones. Within the accuracy limits, the results are in accordance with expectations.

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