Table 3
The 
(fourth column) and rotation periods (fifth column) of the 38 M dwarfs for which both are known.
| Name | V−K | M | log( ) |
P Rot. | P Ref. | P Rot. Fit |
| [mag] | [M⊙] | [d] | [d] | |||
|
|
||||||
| GJ 1264 | 4.288 | 0.74 | –4.055 | 6.67 | (1) | ≤10 |
| Gl 699 | 5.040 | 0.16 | –5.691 | 130 | (1) | 121 |
| Gl 569A | 4.416 | 0.48 | –4.319 | 13.68 | (1) | 15 |
| GJ 182 | 3.680 | 0.79 | –3.859 | 4.41 | (1) | ≤10 |
| GJ 890 | 3.852 | 0.57 | –4.020 | 0.43 | (1) | ≤10 |
| GJ 867A | 4.716 | 0.63 | –4.189 | 4.23 | (1) | 12 |
| GJ 841A | 4.769 | 0.68 | –4.124 | 1.12 | (1) | ≤10 |
| Gl 803 | 4.230 | 0.74 | –3.995 | 4.85 | (1) | ≤10 |
| Gl 729 | 5.080 | 0.17 | –4.428 | 2.87 | (1) | 18 (∗) |
| Gl 618A | 4.686 | 0.38 | –5.401 | 56.52 | (1) | 78 |
| Gl 551 | 6.730 | 0.12 | –5.003 | 82.53 | (1) | 42 |
| GJ 494 | 4.150 | 0.60 | –3.998 | 2.89 | (1) | ≤10 |
| GJ 431 | 4.980 | 0.37 | –4.208 | 14.31 | (1) | 13 |
| GJ 3367 | 3.817 | 0.54 | –4.088 | 12.05 | (1) | ≤10 |
| GJ 1054A | 3.949 | 0.66 | –3.982 | 0.51 | (1) | ≤10 |
| GJ 103 | 3.941 | 0.75 | –4.000 | 1.56 | (1) | ≤10 |
| Gl 205 | 4.080 | 0.63 | –4.599 | 33.61 | (1) | 23 |
| Gl 358 | 4.660 | 0.42 | –4.623 | 25.26 | (1) | 24 |
| Gl 176 | 4.509 | 0.49 | –4.911 | 38.92 | (1) | 37 |
| Gl 674 | 4.480 | 0.34 | –4.885 | 33.29 | (1) | 35 |
| Gl 479 | 4.640 | 0.43 | –4.814 | 23.75 | (2) | 32 |
| Gl 526 | 4.010 | 0.49 | –5.113 | 50.00 | (2) | 50 |
| Gl 388 | 4.710 | 0.42 | –4.191 | 2.24 | (3) | ≤10 |
| Gl 12 | 4.809 | 0.22 | –5.368 | 78.50 | (4) | 74 |
| G 141–29 | 5.235 | 0.24 | –4.400 | 8.07 | (4) | 17 (∗) |
| GJ 3379 | 5.334 | 0.23 | –4.554 | 1.81 | (4) | 21 (∗) |
| GJ 1057 | 5.950 | 0.18 | –5.522 | 102.00 | (4) | 93 |
| LHS 1610 | 5.783 | 0.17 | –5.375 | 78.80 | (4) | 75 |
| Gl 285 | 5.420 | 0.31 | –4.078 | 2.78 | (4) | ≤10 |
| Gl 581 | 4.710 | 0.31 | –5.776 | 130 | (5) | 137 |
| GJ 3293 | 4.520 | 0.52 | –5.114 | 41 | (6) | 50 |
| GJ 3138 | 3.710 | 0.68 | –4.855 | 42 | (7) | 34 |
| Gl 654 | 4.120 | 0.48 | –5.266 | 49 | (7) | 63 |
| Gl 752A | 4.460 | 0.49 | –5.071 | 46 | (7) | 47 |
| Gl 876 | 5.120 | 0.33 | –5.496 | 91 | (7) | 90 |
| Gl 880 | 4.130 | 0.58 | –4.744 | 37 | (7) | 28 |
| Gl 382 | 4.170 | 0.53 | –4.655 | 22 | (7) | 25 |
| Gl 514 | 3.990 | 0.52 | –4.879 | 30 | (7) | 35 |
Notes. References are given in the sixth column: (1) Kiraga & Stepien (2007); (2) Bonfils et al. (2013); (3) Morin et al. (2008); (4) Irwin et al. (2011); (5) Robertson et al. (2014); (6) Astudillo-Defru et al. (2015); and (7) refer to this work. The seventh column gives the rotation periods derived from Eq. (12), where objects flagged with (∗) are the three very-low-mass stars showing the lowest log() in the saturated regime (Fig. 6). The rms of PRot. and PRot. Fit is 12 d. V−K color and stellar mass are tabulated in the second and third columns, respectively.
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