Dust extinction curves: KMH94 R_V=5.5 model
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This dataset is based on the models described in Benson (2018). <strong>Dust Properties</strong> Dust grain properties are taken from Kim, Martin, and Hendry (1994), specifically their model with with R<sub>V</sub>=3.1 and a full scattering calculation. <strong>Stellar Geometry</strong> Galactic disks follow exponential profiles in the radial direction, and sech<sup>2</sup> distributions in the vertical direction. The vertical scale height is set to a multiple, <em>h</em><sub>d</sub>, of the stellar disk scale length, and its value is encoded in each file name. Spheroids follow spherical Hernquist (1990) profiles. <strong>Dust Geometry</strong> Dust is distributed in the disk, and follows exponential profiles in both radial and vertical directions. The vertical scale height is set to a multiple, <em>h</em><sub>z</sub>, of the stellar disk scale length, and its value is encoded in each file name.
