A 0.1339 solar mass object is located at origin and emitting wind. Although parameters change in the following simulations, the functional form of time dependent variables behave alike.

The initial velocity of the wind and The density of the wind vary as:

Red line indicate the escape velocity at the radius where the wind is launched.

\frac{\triangle t}{t_f}	0.5	0.367
	color1.gif​	color4.gif​
	1.gif​	4.gif​
\frac{v_w}{v_{esc}}	0.670	0.768
\frac{\dot{M}_{pulse}v_{pulse}}{\dot{M}_{postp}v_{postp}}	58	29
	color1.gif​	color5.gif​
	1.gif​	5.gif​