On the Orbital Eccentricity of an Eclipsing Binary System

Details On the Orbital Eccentricity of an Eclipsing Binary System On the Orbital Eccentricity of an Eclipsing Binary System

Feb 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..15..229t&link_type=abstract

Astrophysics and Space Science, Volume 15, Issue 2, pp.229-235

Astronomy and Astrophysics

Astrophysics

10

Scientific paper

A new method is presented to precisely deduce the orbital eccentricity
of an eclipsing binary from observed epochs of its light minima.
Application to the system V526 Sagittarii givese=0.2220±0.0016.

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