astronomix._modules._stellar_wind.weaver#
Analytic Weaver et al. (1977) stellar-wind bubble solution.
Provides the Weaver self-similar solution for a wind-blown bubble:
given the wind terminal velocity, mass-loss rate and the ambient ISM density /
pressure, it integrates the shell structure equations and exposes the radial
density, velocity and pressure profiles (free wind, shocked wind interior,
swept-up shell and undisturbed ISM) at a given time.
Module Contents#
Classes#
Weaver et al. (1977) self-similar stellar-wind bubble solution. |
API#
- class astronomix._modules._stellar_wind.weaver.Weaver(v_inf, M_dot, rho_0, p_0, num_xi=100, gamma=5 / 3)[source]#
Weaver et al. (1977) self-similar stellar-wind bubble solution.
Initialised from the wind terminal velocity
v_inf, the mass-loss rateM_dotand the ambient ISM densityrho_0/ pressurep_0; the resulting object yields the density, velocity and pressure profiles of the wind bubble at any timet.Initialization
- calculate_shell_profiles()[source]#
Integrate the self-similar shell structure equations.
Integrates equations 6 to 7 of Weaver II inward from the outer shock (
xi = 1) to the critical radius (xi = xi_crit):3 (U - xi) U’ - 2 U + 3 P’ / G = 0 (U - xi) G’ / G + U’ + 2 U / xi = 0 3 (U - xi) P’ - 3 gamma P (U - xi) G’ / G - 4 P = 0
where a prime denotes a derivative with respect to xi, with boundary conditions G(1) = 4, U(1) = 3/4, P(1) = 3/4. The dimensionless profiles relate to physical quantities by r = R_2 xi, rho = rho_0 G(xi), v = V_2 U(xi) and p = rho_0 V_2^2 P(xi). The results are stored on the instance ordered from the critical radius outward.
- get_radial_range_wind_interior(delta_R, t)[source]#
Return the radial sampling points across the shocked wind interior.
- get_radial_range_free_wind(delta_R, t)[source]#
Return the radial sampling points across the freely expanding wind.
- get_radial_range_undisturbed_ism(delta_R, R_max, t)[source]#
Return the radial sampling points across the undisturbed ISM.
- get_pressure_profile(delta_R, R_max, t)[source]#
Return the radial pressure profile of the wind bubble at time
t.Concatenates the (uniform) shocked-wind-interior pressure, the shell pressure and the undisturbed-ISM pressure, returning the matching radii alongside the pressures.