Theoretical values of convective turnover times and Rossby numbers for solar-like, pre-main sequence stars

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Volume 510 (February 2010)

A&A, 510 (2010) A46

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Table 1:

Pre-main sequence evolutionary tracks (including $\log \tau_{\rm c}$ , $\log\tau_{\rm g}$ and Ro) for 1 $M_{\odot }$ star^a.
$\displaystyle{\log {\rm Age}\atop{\rm (years)}}$	$\displaystyle\log\frac{L}{L_{\odot}}$	$\displaystyle{\log T_{\rm eff}\atop{\rm (K)}}$	$\displaystyle\log g\atop{\displaystyle\rm (cgs)}$	$\displaystyle\log \tau_{\rm c}\atop{\displaystyle\rm (s)}$	$\displaystyle\tau_{\rm g}\atop\rm {\displaystyle(days)}$	Ro
6.2324	0.1468	3.6524	3.855	6.3275	766.6288	0.1436
6.4053	0.0217	3.6513	3.976	7.1018	488.2106	0.0183
6.5840	-0.1029	3.6499	3.095	7.0810	369.1187	0.0146
6.7666	-0.2172	3.6494	4.207	7.0074	291.4590	0.0131
6.9324	-0.2965	3.6522	4.297	6.9087	227.1363	0.0129
7.0786	-0.3278	3.6606	4.362	6.7949	179.1020	0.0135
7.2016	-0.2987	3.6775	4.401	6.6878	134.8216	0.0145
7.2978	-0.2231	3.6999	4.415	6.5727	99.6126	0.0165
7.3740	-0.1262	3.7232	4.411	6.4301	72.7130	0.0204
7.4394	-0.0387	3.7445	4.409	6.2546	53.4192	0.0269
7.5214	-0.0924	3.7525	4.494	6.1771	41.6650	0.0232
7.9918	-0.1590	3.7461	4.536	6.1942	46.0585	0.0212
9.0247	-0.1138	3.7531	4.518	6.1821	42.4793	0.2593
9.3023	-0.0862	3.7553	4.499	6.1523	41.0925	0.7916
9.4669	-0.0580	3.7572	4.479	6.1598	39.4493	1.0789
9.5829	-0.0288	3.7591	4.457	6.1303	38.1493	1.4206
9.6573	-0.0040	3.7605	4.438	6.1369	38.0850	1.5989
9.6980	0.0119	3.7612	4.425	6.1409	37.5359	1.7020
9.7644	0.0428	3.7624	4.399	6.1102	36.8616	2.0771
9.8211	0.0754	3.7634	4.370	6.1166	36.2118	2.3108

^(a) The complete version of the table, including seven tracks for all the masses of Table 2, will be available in electronic form at the CDS.

Source LaTeX | All tables | In the text

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