A Application of WD Model to EB Type Contact Binary System

Details A Application of WD Model to EB Type Contact Binary System A Application of WD Model to EB Type Contact Binary System

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000jass...17..172o&link_type=abstract

Journal of Astronomy and Space Sciences, vol. 17, no. 2, p. 163-172

Astronomy and Astrophysics

Astronomy

Stars, Contact Binary, Light Curves

Scientific paper

The EB type contact binaries show large temperature difference ( T 1,000K) between two components. Thus we have modified the mode 3 of the WD program to adjust albedos, limb darkening coefficients and gravity darkening exponents for both components of such binaries, while the values for those parameters should be same for both components in the original WD program. Both of the modified and the original versions have been applied to the EB type contact binaries such as DO Cas, GO Cyg, and FS Lup. The computed light curves with modified version fit better to the observations.

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