The astro modules and programs¶

Module astro_bin_vero¶

Module : astro_bin_vero

Purpose : Version of centrifugally disorted star to account for phase locked binary.

class star_t¶

class discfunc_t¶

star_t_(m, ar) result (st)¶

Phi_eff_(this, vr) result (Phi_eff)¶

vg_eff_(this, vr) result (vg_eff)¶

vn_eff_(this, vr) result (vn_eff)¶

D_surf_(this, vr) result (D_surf)¶

Sigma_0_(this) result (Sigma_0)¶

Sigma_1_(this) result (Sigma_1)¶

A_surf_(this) result (A_surf)¶

R_surf_(this, theta) result (R_surf)¶

s_surf_(this, vr_0, vdr) result (s_surf)¶

eval_c_(this, z) result (f_z)¶

read_(hg, st)¶

write_(hg, st)¶

bcast_(st, root_rank)¶

Module astro_hough¶

Module : astro_hough

Purpose : calculation of Hough eigenvalues & eigenfunctions, incl. hough_t type

class hough_t¶

hough_t_n_(nu, m, k, n) result (ho)¶

hough_t_tol_(nu, m, k, tol) result (ho)¶

Theta_(this, mu) result (Theta)¶

Theta_xi_(this, mu) result (Theta_xi)¶

Xi_(nu, m, n, parity)¶

J_lm_(l, m)¶

P_lm_series(n, m, x) result (P_lm)¶

dP_lm_series(n, m, x) result (dP_lm)¶

N_lm_series(n, m) result (N_lm)¶

lambda_n_(nu, m, k, n) result (lambda)¶

lambda_tol_(nu, m, k, tol) result (lambda)¶

lambda_asymp(nu, m, k) result (lambda)¶

lambda_3(nu, m, k) result (lambda)¶

eval_coeffs_(nu, m, k, lambda, b, c_r, c_t, c_p)¶

eval_eigvecs_(nu, m, k, lambda, b, q, r)¶

eigen_W_n_(nu, m, k, n, lambda, b)¶

eigen_W_tol_(nu, m, k, tol, lambda, b)¶

eigen_A_i_(nu, m, parity, n, i, k, lambda, b)¶

eval_A_(nu, m, n, parity, A_D, A_E)¶

assemble_A_(nu, m, n, parity, A_1, A_2n, A_2d, A_3n, A_3d, A_4n, A_4d, A_5, A_D, A_E)¶

save_ieee_state_(h_over, h_zero, h_inval)¶

restore_ieee_state_(h_over, h_zero, h_inval)¶

Module astro_orbit¶

Module : astro_orbit

Purpose : binary orbits

class orbit_t¶

class lagrange_func_t¶

phase_(this, t, t_peri) result (phase)¶

a_(this, star) result (a)¶

rho_(this, upsilon, star) result (rho)¶

rho_dot_(this, upsilon, star) result (rho_dot)¶

r_(this, phase, star) result (r)¶

r_dot_(this, phase, star) result (r_dot)¶

upsilon_(this, phase, star) result (upsilon)¶

E_5_(e, M) result (E_5)¶

upsilon_dot_(this, phase, star) result (upsilon_dot)¶

vr_(this, phase, star) result (vr)¶

vv_(this, phase, star) result (vv)¶

vr_L_(this, phase, i) result (vr_L)¶

eval_c_(this, z) result (f_z)¶

lagrange_force(lf, x) result (f)¶

Module astro_star¶

Module : astro_star

Purpose : centrifugally disorted star

class star_t¶

class discfunc_t¶

star_t_(omega) result (st)¶: Testing the docstrings Another line of doc string Here’s the more complete description that continues on another line

Phi_eff_(this, vr) result (Phi_eff)¶

Calculate the effective potential (units: G M_star/R_pole) at vr (units: R_pole)

Parameters

this – a star_t object
vr – a position

Rtype Phi_eff

the potential as position vr

vg_eff_(this, vr) result (vg_eff)¶

vn_eff_(this, vr) result (vn_eff)¶

D_surf_(this, vr) result (D_surf)¶

Sigma_0_(this) result (Sigma_0)¶

Sigma_1_(this) result (Sigma_1)¶

A_surf_(this) result (A_surf)¶

R_surf_(this, theta) result (R_surf)¶

s_surf_(this, vr_0, vdr) result (s_surf)¶

eval_c_(this, z) result (f_z)¶

read_(hg, st)¶

write_(hg, st)¶

bcast_(st, root_rank)¶