Models for the Spectral Energy Distibution of Disks at Long Wavelengths

Details Models for the Spectral Energy Distibution of Disks at Long Wavelengths Models for the Spectral Energy Distibution of Disks at Long Wavelengths

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21542806g&link_type=abstract

American Astronomical Society, AAS Meeting #215, #428.06; Bulletin of the American Astronomical Society, Vol. 42, p.345

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We discuss the spectral energy distributions (SEDs) of axisymmetric circumstellar disks that produce infrared (IR), millimeter (mm), and radio emission excesses. In particular, we explore the effects of disk flaring on the SED shape. We find that relatively mild deviations from a power-law SED result from flaring. Key diagnostics for assessing flared disks from the SEDs are highlighted, and applications to IR and mm spectral measurements for Be star disks are noted.
This research was funded by a grant from the National Science Foundation, AST-0936427.

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