The core helium flash revisited - III. From Population I to Population III stars

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Table 2:

Some properties of the 3D simulation based on model M.
Run	Grid	w	$\Delta r$	$\Delta\theta$	$\Delta\phi$	$R_{\rm e}$	$v_{\rm c}$	$\tau_{\rm cnv}$	$t_{\max}$
$\mbox{[name]}$	$N_{\rm r} \times N _\theta \times N_\phi$	[ $\mbox{$^\circ$ }$ ]	[10⁶ cm]	[ $\mbox{$^\circ$ }$ ]	[ $\mbox{$^\circ$ }$ ]		[10 $^{6}~\mbox{\ cm~s${}^{-1}$ }$ ]	[s]	[s]
heflpopI.3d	$270\times30\times30$	30	3.7	1	1	10²	1.1	1000	100 000

Notes. Number of grid zones, wedge size w, grid resolution in r, $\theta$ and $\phi$ direction, estimated Reynolds number $R_{\rm e}$ (Porter & Woodward 1994), approximate characteristic velocity $v_{\rm c}$ of the convective flow, typical convective turnover timescale $\tau_{\rm cnv}$ , and maximum evolutionary time $t_{\max}$ .

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