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) |
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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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