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http://hea-www.harvard.edu/~swolk/thesis/node91.html.
http://hea-www.harvard.edu/~swolk/thesis/node91.html.
1. Eclipse Lightcurves for the Hydrostatic Model
Next: Disk Expansion and Up: The Epsilon Aurigae Previous: Vertical Structure of . ... We model disks with and without central holes and use a variety of midplane opacities and temperatures. ... The eclipse lightcurve was computed on a grid of 505 time steps separated by approximately 1.3 days, for a range of values of the disk scale height, , the inclination, i , and central hole radius, . The opacity parameter, approximately equal to the ``vertical'' optical depth of the disk, is: . ...
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Ссылки http://hea-www.harvard.edu/~swolk/thesis/node90.html -- 18.5 Кб -- 01.10.2012
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