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Table 1

Pre-main sequence evolutionary tracks for 0.4 M star for disk-locking models with Plock = 5 days and Tdisk = 1 Myr(a).

log Age(years) log Teff(K) log Itot(cgs) log Iconv(cgs) Prot(days)

2.6990 1.1983 3.5364 1.000 55.8939 55.8939 5.000
3.7669 0.8332 3.5731 1.000 55.4176 55.4176 5.000
4.3476 0.6145 3.5792 1.000 55.1964 55.1964 5.000
4.7922 0.3949 3.5801 1.000 54.9815 54.9815 5.000
5.6514 0.1908 3.5778 1.000 54.7917 54.7917 5.000
5.8159 0.0243 3.5726 1.000 54.6489 54.6489 5.000
5.9375 0.1792 3.5615 1.000 54.4934 54.4934 5.000
6.1166 0.3993 3.5479 1.000 54.3315 54.3315 3.939
6.3691 0.6192 3.5404 1.000 54.1459 54.1459 2.569
6.6674 0.8394 3.5367 1.000 53.9446 53.9446 1.616
6.9887 1.0597 3.5353 1.000 53.7342 53.7342 0.996
7.3155 1.2801 3.5342 0.968 53.5215 53.5208 0.610
7.6562 1.4993 3.5341 0.758 53.3016 53.2757 0.368
8.0368 1.6855 3.5380 0.486 53.0810 52.9713 0.221
10.0536 1.7186 3.5372 0.520 53.0592 52.9586 0.210
10.5776 1.6919 3.5388 0.474 53.0648 52.9477 0.213
10.8272 1.6613 3.5410 0.427 53.0680 52.9327 0.215
10.9838 1.6247 3.5438 0.384 53.0713 52.9176 0.216
11.0939 1.5809 3.5474 0.346 53.0757 52.9065 0.219
11.1772 1.5275 3.5518 0.312 53.0822 52.8996 0.222

Notes. Column 1 gives the logarithm of stellar age (years); Col. 2 the logarithm of stellar luminosity (solar units); Col. 3 the logarithm of effective temperature (K); Col. 4 the mass contained in the convective envelope relative to the total mass (Mconv/Mtot); Col. 5 the logarithm of total rotational inertia (log Itot, cgs); Col. 6 the logarithm of rotational inertia in the convective envelope (log Iconv, cgs); and Col. 7 the rotational period (Prot, days).

(a) The complete version of the table, including 40 tracks for 0.15, 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, and 0.8 M for models considering both conservation of angular momentum and disk-locking (with locking period of 5 and 8 days and disk lifetimes of 0.5 and 1 Myr) is available at the CDS.

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