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[ascl:2002.022] DISKMODs: Accretion Disk Radial Structure Models

DISKMODs provides radial structure models of accretion disk solutions. The following models are included: Novikov-Thorne thin disk model and Sadowski polytropic slim disk model. Each model implements a common interface that gives the radial dependence of selected geometrical, physical and thermodynamic quantities of the accretion flow. The model interpolates through a set of tabulated numerical solutions. These solutions are computed for a reference mass M=10 Msun. The model can rescale the disk structure to any mass, with masses in the range of 5-20 Msun giving reasonably good results.

Code site:
https://github.com/mbursa/disk-models
Described in:
https://ui.adsabs.harvard.edu/abs/2011A%26A...527A..17S
Bibcode:
2020ascl.soft02022B
Preferred citation method:

https://ui.adsabs.harvard.edu/abs/2020ascl.soft02022B ; please see additional citation information here: https://github.com/mbursa/disk-models#citing


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ascl:2002.022
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