Table 1: Parameters for the two- and three-dimensional runs.
Fig. # 3 (top-row) 3 (bottom-row) 5

$n_{\rm e}$ ( $\mbox{cm}^{-3}$ ) 10⁵ 10⁶ 10⁵

$T_{\rm e}$ ( $\mbox{K}$ ) 500 5000 500

$n_{\rm d}$ ( $\mbox{cm}^{-3}$ ) 10⁷ 10⁸ 10⁷

$T_{\rm d}$ ( $\mbox{K}$ ) 5 50 5

$\dot{M}_{\rm w}$ ( $M_\odot~\mbox{yr}^{-1}$ ) $1.7\times 10^{-9}$ $1.7\times 10^{-8}$ $1.7\times 10^{-9}$

$R_{\rm crit}$ (AU) 18 18 18

$t_{\rm p}$ ( $\mbox{yr}$ ) >890 >890 >890

$t_{\rm sp}$ ( $\mbox{yr}$ ) 15 15 15

$t_{\rm c,A}$ ( $\mbox{yr}$ ) 5.8 0.58 5.8

$t_{\rm c,B}$ ( $\mbox{yr}$ ) $2.0\times 10^{-5}$ $2.0\times 10^{-6}$ $2.0\times 10^{-5}$

**Table 1:** Parameters for the two- and three-dimensional runs.
Fig. #	3 (top-row)	3 (bottom-row)	5
$n_{\rm e}$ ( $\mbox{cm}^{-3}$ )	10⁵	10⁶	10⁵
$T_{\rm e}$ ( $\mbox{K}$ )	500	5000	500
$n_{\rm d}$ ( $\mbox{cm}^{-3}$ )	10⁷	10⁸	10⁷
$T_{\rm d}$ ( $\mbox{K}$ )	5	50	5
$\dot{M}_{\rm w}$ ( $M_\odot~\mbox{yr}^{-1}$ )	$1.7\times 10^{-9}$	$1.7\times 10^{-8}$	$1.7\times 10^{-9}$
$R_{\rm crit}$ (AU)	18	18	18
$t_{\rm p}$ ( $\mbox{yr}$ )	>890	>890	>890
$t_{\rm sp}$ ( $\mbox{yr}$ )	15	15	15
$t_{\rm c,A}$ ( $\mbox{yr}$ )	5.8	0.58	5.8
$t_{\rm c,B}$ ( $\mbox{yr}$ )	$2.0\times 10^{-5}$	$2.0\times 10^{-6}$	$2.0\times 10^{-5}$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Point-symmetric nebulae
	3 Radiation driven warping
	4 Time scales
	5 Numerical implementation
	6 Two-dimensional wind-disk simulations
	7 Mechanism
	8 Three-dimensional wind-disk simulations
	9 Conclusions
	References
	Online Material