Orbital Solutions and Absolute Elements of the Eclipsing Binary AR Mon

Details Orbital Solutions and Absolute Elements of the Eclipsing Binary AR Mon Orbital Solutions and Absolute Elements of the Eclipsing Binary AR Mon

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.1204w&link_type=abstract

American Astronomical Society Meeting 203, #12.04; Bulletin of the American Astronomical Society, Vol. 35, p.1222

Astronomy and Astrophysics

Astronomy

Scientific paper

Differential UBV photoelectric photometry has been obtained for the binary AR Mon during four consecutive seasons. This system is one of only a few that consists of two late-type evolved stars. The period is 21.2 days. The Wilson-Devinney program is used to simultaneously solve three, combined-data light curves with previously published radial velocities. Two solutions are presented -- a 98% lobe-filling solution and a 100% (semi-detached) solution. New absolute dimensions are calculated.

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