The impact of disk-locking on convective turnover times of low-mass pre-main sequence and main sequence stars

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Volume 693 (January 2025)

A&A, 693 (2025) A68

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Table 1.

Evolutionary track for 1 M_⊙ star (DL model with P_lock ∼ 8 days and T_disk = 3 Myr).

$\log \frac{t}{yr}$ $\mathrm{log}\frac{t}{\mathrm{yr}}$	$\log \frac{L}{L_{⊙}}$ $\mathrm{log}\frac{L}{L_\odot}$	log(T_eff/K)	log(g/cm s⁻²)	log(τ_c/d)	log(τ_g/d)	P_rot/d	Ro	M_rad(M_⊙)
2.233	1.665	3.600	2.127	1.976	2.910	10.580	0.112	0.000
3.668	1.601	3.623	2.280	1.901	2.805	10.580	0.133	0.000
4.203	1.382	3.634	2.545	1.892	2.792	10.580	0.136	0.000
4.643	1.163	3.642	2.795	1.874	2.708	10.580	0.141	0.000
5.186	0.989	3.647	2.989	1.871	2.687	10.580	0.143	0.000
5.352	0.836	3.651	3.158	1.870	2.781	10.580	0.143	0.000
5.606	0.615	3.653	3.389	1.869	2.785	10.580	0.143	0.000
5.882	0.394	3.652	3.604	1.873	2.810	10.580	0.142	0.000
6.164	0.173	3.646	3.802	1.942	2.853	10.580	0.121	0.003
6.454	–0.048	3.637	3.987	2.144	2.589	10.580	0.076	0.160
6.779	–0.253	3.632	4.173	2.059	2.406	6.859	0.060	0.428
7.054	–0.316	3.650	4.305	1.893	2.211	4.469	0.057	0.680
7.248	–0.221	3.689	4.367	1.683	1.990	3.020	0.063	0.853
7.372	–0.049	3.734	4.376	1.439	1.756	2.082	0.076	0.946
7.478	0.019	3.766	4.437	1.177	1.504	1.418	0.094	0.983
8.563	–0.092	3.759	4.520	1.213	1.521	1.354	0.083	0.980
9.277	–0.043	3.764	4.487	1.187	1.500	1.363	0.089	0.982
9.490	–0.001	3.767	4.458	1.178	1.481	1.372	0.091	0.984
9.624	0.040	3.769	4.427	1.150	1.460	1.389	0.098	0.985
9.743	0.094	3.772	4.384	1.142	1.443	1.423	0.103	0.986

Notes. Column 1 gives the log₁₀ of stellar age; Col. 2 the log₁₀ of bolometric luminosity; Col. 3 the log₁₀ of effective temperature; Col. 4 the log₁₀ of effective gravity; Col. 5 the log₁₀ of local convective turnover time; Col. 6 the log₁₀ of global convective turnover time; Col. 7 the rotation period; Col. 8 the Rossby number; and Col. 9 the radiative core mass. Throughout this work all the logarithms are in base 10.

The complete version of the table, including 24 tracks for masses in the range 0.1–1.2 M_⊙ (in 0.1 M_⊙ increments) for DL and AMC models, is available at the CDS.

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