peebee.models Module¶
Peebee contains many different potential models, which can be used to either generate acceleration data, or can be fit to existing acceleration data. A variety of models are incorporated here, and are added as they become relevant. If you do not see a specific potential you are interested in, you can reach out and ask that it be added to a future version of peebee.
Classes¶
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Anharmonic disk model with polynomial vertical expansion. |
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Cox & Gomez (2002) spiral arm potential model. |
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Cross model for Galactic dynamics. |
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Damour-Taylor numerical potential model. |
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Exponential disk model (NOT a double exponential disk!). |
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Wrapper for Gala potential objects. |
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Generic Galpy potential wrapper. |
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Hernquist spherical mass profile. |
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Isothermal disk model with constant velocity dispersion. |
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Isothermal disk with beta parameter for rotation curve slope. |
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Local expansion model with acceleration gradients. |
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Base class for gravitational potential models. |
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Navarro-Frenk-White (NFW) dark matter halo profile. |
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Miyamoto-Nagai disk with vertical offset. |
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Oort expansion (alpha) model with flexible vertical and radial components. |
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Plummer sphere mass distribution. |
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Point mass gravitational source. |
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Radial density oscillation model. |
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Sinusoidal disk model with oscillatory vertical structure. |
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Spherical potential with flat rotation curve. |
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Uniform 3D acceleration model. |
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Uniform line-of-sight acceleration model. |