Two-component jet simulations - II. Combining analytical disk and stellar MHD outflow solutions

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Volume 502 / No 1 (July IV 2009)

A&A, 502 1 (2009) 217-229

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Table 3:

The time variable numerical models.
Name	$T_{\rm var}/T_{\rm K}$	Variability	Variable wind	Description
1-S1	1	V_z	Stellar	Very high frequency velocity fluctuations of the stellar component (Fig. 11)
2-S10	10	V_z	Stellar	High frequency velocity fluctuations of the stellar component
3-S10²	10²	V_z	Stellar	Medium frequency velocity fluctuations of the stellar component (Figs. 11, 12)
4a-S10³	10³	V_z	Stellar	Low frequency velocity fluctuation of the stellar component (Fig. 14)
4b-S10³	10³	V_z	Stellar	Low freq. vel. fluct. (lower magnitude: $\pm20\%$ ) of the stellar component (Fig. 14)
5-S10⁴	10⁴	V_z	Stellar	Very low frequency velocity fluctuations of the stellar component (Fig. 14)
6-X1	1	$V_z~\&~\rho$	X-type	Very high frequency momentum fluctuations around the X-point (Fig. 13)
7-X10	10	$V_z~\&~\rho$	X-type	High frequency momentum fluctuations around the X-point
8-X10²	10²	$V_z~\&~\rho$	X-type	Medium frequency momentum fluctuations around the X-point (Fig. 13)

The two-component jet parameters are the same for all cases: $\ell_l = 0.1$ , $\ell_V = 5.96$ , $\ell_B = 2.0$ , $A_{\rm m} = 1.33$ , q = 0.2 and d = 2.0.

Source LaTeX | All tables | In the text

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