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Attenuation curves are described by 3 physical parameters:
optical depth
Rs / Rd: ratio of radii for stellar and dust distributions
Mach number : governing the variance of the ISM density field , i.e. quantifying the
clumpiness of the ISM (Ms=0 for homogeneous , Ms=20 for very clumpy and turbulent medium)
Aim: make interpolation between the discretized values.
The text was updated successfully, but these errors were encountered:
Add in the attenuation curves from the radiative transfer simulations of Seon 2016
http://adsabs.harvard.edu/abs/2016ApJ...833..201S
Publicly available here: https://seoncafe.github.io/MoCafe.html
Attenuation curves are described by 3 physical parameters:
clumpiness of the ISM (Ms=0 for homogeneous , Ms=20 for very clumpy and turbulent medium)
Aim: make interpolation between the discretized values.
The text was updated successfully, but these errors were encountered: