Apsidal motion in the eclipsing binary FT Orionis.

Details Apsidal motion in the eclipsing binary FT Orionis. Apsidal motion in the eclipsing binary FT Orionis.

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26as..114..143w&link_type=abstract

Astronomy and Astrophysics Supplement, v.114, p.143

Astronomy and Astrophysics

Astrophysics

15

Binaries: Eclipsing, Stars: Individual: Ft Ori

Scientific paper

We report several new photoelectric times of minimum for the eclipsing
binary FT Orionis with large orbital eccentricity. They confirm the
existence of a periastron revolution. Using all precise timings found in
the literature, new values for the elements of the apsidal motion and
the internal structure constant are computed.

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