Dust extinction curves: KMH94 R_V=5.5 model

<p>This dataset is based on the models described in <a href="https://ui.adsabs.harvard.edu/abs/2018RNAAS...2..188B">Benson (2018)</a>.</p> <p><strong>Dust Properties</strong></p> <p>Dust grain properties are taken from <a href="http://adsabs.harvard.edu/abs/1994ApJ...422..164K">Kim, Martin, and Hendry (1994)</a>, specifically their model with with R_V=3.1 and a full scattering calculation.</p> <p><strong>Stellar Geometry</strong></p> <p>Galactic disks follow exponential profiles in the radial direction, and sech² distributions in the vertical direction. The vertical scale height is set to a multiple, <em>h</em>_d, of the stellar disk scale length, and its value is encoded in each file name. Spheroids follow spherical <a href="http://adsabs.harvard.edu/abs/1990ApJ...356..359H">Hernquist (1990)</a> profiles.</p> <p><strong>Dust Geometry</strong></p> <p>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>_z, of the stellar disk scale length, and its value is encoded in each file name.</p>