galpy.df.impulse_deltav_general_fullplummerintegration

galpy.df.impulse_deltav_general_fullplummerintegration(v, x, b, w, x0, v0, galpot, GM, rs, tmaxfac=10.0, N=1000, integrate_method='symplec4_c')[source]

Calculate the delta velocity to due an encounter with a moving Plummer sphere and galactic potential relative to just in galactic potential by integrating each particle in the underlying galactic potential; allows for arbitrary velocity vectors and arbitrary shaped streams.

Parameters:

  • v (numpy.ndarray) – velocity of the stream (nstar,3)

  • x (numpy.ndarray) – position along the stream (nstar,3)

  • b (float) – impact parameter

  • w (numpy.ndarray) – velocity of the subhalo (3)

  • x0 (numpy.ndarray) – position of closest approach

  • v0 (numpy.ndarray) – velocity of point of closest approach

  • galpot (Potential object or list thereof) – galpy Potential object or list thereof

  • GM (float) – mass of Plummer

  • rs (float) – scale of Plummer

  • tmaxfac (float) – multiple of rs/fabs(w - v0) to use for time integration interval

  • N (int) – number of forward integration points

  • integrate_method (str) – orbit integrator to use (see Orbit.integrate)

Returns:

velocity kick deltav (nstar,3)

Return type:

numpy.ndarray

Notes

  • 2015-08-18 - Written - Sanders (Cambridge)