VariableXBarFlow
- class dysmalpy.models.VariableXBarFlow(vbar=None, **kwargs)[source]
Bases:
HigherOrderKinematicsPerturbation
,_DysmalFittable3DModel
- Model for flow along a bar, along some axis in the galaxy midplane,
with flow velocity that varies with bar distance abs(xbar) (under reflection symmetry).
- Parameters:
Notes
The following function must also be passed when setting up the model, which takes the bar coordinate xbar as an input:
vbar(xbar, model_set) [Amplidute of flow velocity as a function of bar coordinate abs(xbar). vbar > 0 for outflow, vbar < 0 for inflow.]
Attributes Summary
Names of the parameters that describe models of this type.
Methods Summary
evaluate
(x, y, z, phi, bar_width, model_set)Evaluate the bar velocity amplitude as a function of position x, y, z
vel_direction_emitframe
(x, y, z[, _save_memory])Method to return the velocity direction in the galaxy Cartesian frame.
velocity
(x, y, z, model_set, *args)Return the velocity as a function of x, y, z
Attributes Documentation
- bar_width = DysmalParameter('bar_width', value=2.0, bounds=(0.0, None), prior=<dysmalpy.parameters.UniformPrior object>)
- outputs = ('vflow',)
- param_names = ('phi', 'bar_width')
Names of the parameters that describe models of this type.
The parameters in this tuple are in the same order they should be passed in when initializing a model of a specific type. Some types of models, such as polynomial models, have a different number of parameters depending on some other property of the model, such as the degree.
When defining a custom model class the value of this attribute is automatically set by the
Parameter
attributes defined in the class body.
- phi = DysmalParameter('phi', value=90.0, bounds=(0.0, 360.0), prior=<dysmalpy.parameters.UniformPrior object>)
Methods Documentation
- evaluate(x, y, z, phi, bar_width, model_set)[source]
Evaluate the bar velocity amplitude as a function of position x, y, z
- vel_direction_emitframe(x, y, z, _save_memory=False)[source]
Method to return the velocity direction in the galaxy Cartesian frame.
- Parameters:
x (float or array) – xyz position in the galaxy/bar reference frame.
y (float or array) – xyz position in the galaxy/bar reference frame.
z (float or array) – xyz position in the galaxy/bar reference frame.
_save_memory (bool, optional) – Option to save memory by only calculating the relevant matrices (eg during fitting). Default: False
- Returns:
vel_dir_unit_vector – Direction of the velocity vector in (xyz).
For a bar uniform flow, this is the sign(xbar) direction, in cartesian coordinates.
- Return type:
3-element array