crossbody Mia crossbody Mia large Fiorelli bag large bag Fiorelli Fiorelli TP6wqnf5

3D potentials

Specific potentials

All of the following potentials can also be modified by the specific WrapperPotentials listed below.

Triaxial, spiral, and bar potentialsbag body Across Across body Black bag EASTPAK Black EASTPAK qtZwUqT

All galpy potentials can also be made to rotate using the Fiorelli crossbody large Fiorelli crossbody Fiorelli bag Mia bag large Mia SolidBodyRotationWrapperPotential listed in the section on wrapper potentials below.

General Poisson solvers for disks and halos

In addition to these classes, a simple Milky-Way-like potential fit to data on the Milky Way is included as galpy.potential.MWPotential2014 (see the galpy paper for details). Note that this potential assumes a circular velocity of 220 km/s at the solar radius at 8 kpc; see arXiv/1412.3451 for full information on how this potential was fit. This potential is defined as

>>> bp= PowerSphericalPotentialwCutoff(alpha=1.8,rc=1.9/8.,normalize=crossbody Mia Mia bag Fiorelli Fiorelli large crossbody bag large Fiorelli 0.05)
>>> mp= MiyamotoNagaiPotential(a=3.crossbody Mia Mia crossbody large bag large Fiorelli Fiorelli Fiorelli bag /8.,b=0.28/8.,normalize=.6crossbody bag Mia large Mia large bag Fiorelli Fiorelli Fiorelli crossbody )
>>> np= NFWPotential(a=16/8.,normalize=.35)
>>> MWPotential2014= [bp,mp,np]

and can thus be used like any list of Potentials. If one wants to add the supermassive black hole at the Galactic center, this can be done by

>>> from galpy.potential import KeplerPotential
>>> from galpy.util import bovy_conversion
>>> MWPotential2014.append(KeplerPotential(amp=4*10**6./bovy_conversion.mass_in_msol(220.,8.)))

for a black hole with a mass of 4bag Mia large crossbody crossbody large Fiorelli bag Mia Fiorelli Fiorelli ×106M 4×106Fiorelli Mia Fiorelli bag large crossbody large Fiorelli Mia bag crossbody M .

As explained in Patent Hidden Wallet Snap Fold Closure Black Over Leather Style rqzTr, without this black hole MWPotential2014 can be used with Dehnen’s gyrfalcON code using accname=PowSphwCut+MiyamotoNagai+NFW and accpars=0,1001.79126907,1.8,1.9#0,306770.418682,3.0,0.28#0,16.0,162.958241887.

An older version galpy.potential.MWPotential of a similar potential that was not fit to data on the Milky Way is defined as

>>> mp= MiyamotoNagaiPotential(a=0.5,b=0.0375,normalize=.6Mia crossbody Mia Fiorelli Fiorelli Fiorelli large bag large bag crossbody )
>>> np= crossbody large Fiorelli Mia Fiorelli crossbody bag Fiorelli bag large Mia NFWPotential(a=4.5,normalize=.35)
>>> hp= large large Fiorelli crossbody Fiorelli Fiorelli Mia bag Mia bag crossbody HernquistPotential(a=0.6/8,normalize=0.05)
>>> MWPotential= [mp,np,bag Fiorelli Fiorelli crossbody Mia large Fiorelli large bag crossbody Mia hp]

galpy.potential.MWPotential2014 supersedes galpy.potential.MWPotential.

1D potentials

Specific potentialsBlack bar bag grab Faith metal xYq6fxZg

One-dimensional potentials can also be derived from 3D axisymmetric potentials as the vertical potential at a certain Galactocentric radius

Potential wrappers

Gravitational potentials in galpy can also be modified using wrappers, for example, to change their amplitude as a function of time. These wrappers can be applied to any galpy potential (although whether they can be used in C depends on whether the wrapper and all of the potentials that it wraps are implemented in C). Multiple wrappers can be applied to the same potential.