A Study of Four Contact Binary Systems Using the DDO Photometric System

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Complete light curves and colour index curves on the DDO photometric system are presented for the W-type contact binary systems W UMa, XY Leo, TX Cnc and AH Vir. The data have been analysed using Rucinski's light curve synthesis code under a variety of constraints. it is found that the gravity darkening exponent must be small (β ≃ 0.00) for these late-type stars (F8-K2). it then follows that the degree of contact between the components is of the order of 25 per cent, rather than the 15 per cent derived if Lucy's value of β =0.08 is adopted, and that there is some indication that the discrepancy between photometric and spectroscopic mass ratios is reduced when β = 0.00 is used.
The significant asymmetries in the light curves of W UMa and AH Vir observed at this epoch may be readily understood in terms of starspots of small extent (≲ 10 per cent of the visible surface of one component).

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