On Light Curves Modeling of Low Inclination Binary Systems with Accretion Disks

Details On Light Curves Modeling of Low Inclination Binary Systems with Accretion Disks On Light Curves Modeling of Low Inclination Binary Systems with Accretion Disks

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aca....48..373z&link_type=abstract

Acta Astronomica, v.48, pp. 373-382, (1998).

Astronomy and Astrophysics

Astronomy

1

Binaries: Close, Accretion: Accretion Disks

Scientific paper

Computer generated light curves of a low inclination, semidetached binary system containing an accretion disk, were analyzed with the Wilson-Devinney code (which does not account for the disk effects), to search for the best solution. The following inclinations were considered: 77 arcdeg 4, 75 arcdeg 0 and 60 arcdeg 0 as well as three different disk contributions to the total light: 2%, 15% and 30%. For the disk contribution being small (2%), the resulting configuration agreed with the input one. For higher disk light detached geometry was derived. The parameters obtained from modeling greatly differ from the input ones and the fits are quite good.

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