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

M. Mocák; S. W. Campbell; E. Müller; K. Kifonidis

doi:10.1051/0004-6361/201014461

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Volume 520 (September-October 2010)

A&A, 520 (2010) A114

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Table 4:

Some properties of the 2D and 3D hydrodynamic models based on initial model SC.
Run	Grid	w	$\Delta r$	$\Delta\theta$	$\Delta\phi$	$R_{\rm e1}$	$R_{\rm e2}$	$v_{\rm c1}$	$v_{\rm c2}$	$\tau_{\rm cnv1}$	$\tau_{\rm cnv2}$	$t_{\rm max}$
$\mbox{[name]}$	$N_{\rm r} \times N_\theta \times$ N $_\phi$	[ $\mbox{$^\circ$ }$ ]	[10⁶ cm]	[ $\mbox{$^\circ$ }$ ]	[ $\mbox{$^\circ$ }$ ]			[ $10^{6}~\mbox{\ cm~s${}^{-1}$ }$ ]	[ $10^{6}~\mbox{\ cm~s${}^{-1}$ }$ ]	[ s ]	[ s ]	[ s ]
heflpopIII.2d.1	$720 \times 50$	50	7.6	1	-	10³	10²	1.3	1.0	2900	2400	1400
heflpopIII.2d.2	$1500 \times 120$	120	3.7	1	-	10⁵	10³	1.7	1.0	2200	2400	6400
heflpopIII.3d	$720 \times 50 \times 50$	50	7.6	1	1	10²	10²	0.4	0.3	9500	8000	1400

Notes. Number of grid zones, wedge size w, grid resolution in r, $\theta$ and $\phi$ direction, estimated Reynolds numbers $R_{\rm e1}$ , $R_{\rm e2}$ , characteristic flow velocities, $v_{\rm c1}$ and $v_{\rm c2}$ , and typical convective turnover timescales, $\tau_{\rm cnv1}$ and $\tau_{\rm cnv2}$ , for the CVZ-1 and CVZ-2 part of the convection zone, respectively. $t_{\rm max}$ is the maximum evolution time.

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