The Third Light in the Eclipsing System with the Apsidal Motion Co-Lacertae

Details The Third Light in the Eclipsing System with the Apsidal Motion Co-Lacertae The Third Light in the Eclipsing System with the Apsidal Motion Co-Lacertae

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987atsir1495....5m&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1495/JUN, 1987

Astronomy and Astrophysics

Astronomy

4

Scientific paper

The determination of the photometric elements of the eclipsing binary
system with apsidal motion by the iterative least squares method allows
to state the presence of a third body in this system (L3 =
0.07). The absolute elements and the apsidal parameter k2 are
redetermined.

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