Titlebook: Light Curve Modeling of Eclipsing Binary Stars; E. F. Milone Conference proceedings 1993 Springer-Verlag New York, Inc. 1993 Periastron.Va

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Spectral Energy Distributions of Circumstellar Gas in Algols,ists of four separable parts: (1) gas flow, (2) radiative properties, in particular, emission line strengths and profiles, (3) generation of spectral energy distributions by spatial integration with Doppler shifts and eclipses, and (4) adjustment of model parameters based on comparisons with observa

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Binary Star Rotation from Line Profiles,pe binaries is mainly a consequence of mass transfer, and thus can provide evolutionary information. Also, rotation is a neglected area of stellar astronomy, especially on the observational side, and it is appropriate to develop our knowledge simply because unexpected benefits nearly always accompan

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Improvements to the Wilson-Devinney Code on Computer Platforms at the University of Calgary, has concentrated on the atmospheres option in the Wilson-Devinney program, the uniqueness determination question, and code portability. We also describe a number of useful tools to facilitate adjustments and the examination of results and consider areas for further development.

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New Atmospheres for Modelling Binaries and Disks,pacities for the temperature range 2000K to 200000K. Calculations have been completed at the San Diego Supercomputer Center for 56 temperatures, for 21 pressures, for microturbulent velocities 0, 1, 2, 4, and 8 km/s, for 3,500,000 wavelength points divided into 1221 intervals from 10 to 10000 nm, fo

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Light Synthesis Modeling of Close Binary Stars,omponents, from the canonical Roche model. Examples of observed departures include the O’Connell effect and ”anomalies” in W Ursae Majoris systems..The simulation of these residual effects requires a flexible program package, and involves the introduction of additional parameters, some of which may

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