We present theoretical infrared images for Be star disks as projected on the plane of the sky. These images span a range of Be star spectral types and a wide range of disk properties and viewing inclinations. We extract the sizes of these disks at different IR wavelengths. As a test of these images, we compare our calculated disk sizes with available interferometric observations of the Be stars α Ara and ζ Tau. We use our calculated disk sizes and the observations to constrain the disk parameters of these stars.
Hamed, G. E., & Sigut, T. (2013). Theoretical infrared continuum images for Be star disks. NRIAG Journal of Astronomy and Geophysics, 2(1), 125-133. doi: 10.1016/j.nrjag.2013.06.015
MLA
Gamal Edin Hamed; T.A.A. Sigut. "Theoretical infrared continuum images for Be star disks", NRIAG Journal of Astronomy and Geophysics, 2, 1, 2013, 125-133. doi: 10.1016/j.nrjag.2013.06.015
HARVARD
Hamed, G. E., Sigut, T. (2013). 'Theoretical infrared continuum images for Be star disks', NRIAG Journal of Astronomy and Geophysics, 2(1), pp. 125-133. doi: 10.1016/j.nrjag.2013.06.015
VANCOUVER
Hamed, G. E., Sigut, T. Theoretical infrared continuum images for Be star disks. NRIAG Journal of Astronomy and Geophysics, 2013; 2(1): 125-133. doi: 10.1016/j.nrjag.2013.06.015
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