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Table 5.
Comparison of the rotation periods given in the literature with our measured values for the early-M stars.
Reference | Category | Gl 205 | Gl 382 | Gl 410 | Gl 514 | Gl 846 | Gl 880 |
---|---|---|---|---|---|---|---|
This work | Bℓ | 34.3 ± 0.4 | 21.32 ± 0.04 | 13.87 ± 0.08 | 30.45 ± 0.14 | 11.01 ± 0.20 | 37.7 ± 0.7 |
Kiraga & Stepien (2007) | phm | 33.61 | 21.56 | ||||
Donati et al. (2008) | ZDI | 14.0 | |||||
Bonfils et al. (2013) | act | 32.8, 39.3 | 10.7 | ||||
Suárez Mascareño et al. (2015) | act | 35.0 ± 0.1 | 21.7 ± 0.1 | 28.0 ± 2.9 | 31.0 ± 0.1 | 37.5 ± 0.1 | |
Suárez Mascareño et al. (2016) | phm | 33.4 ± 0.1 | 21.2 ± 0.1 | ||||
Hébrard et al. (2016) | ZDI | 33.63 ± 0.37 | 13.83 ± 0.10 | 10.73 ± 0.10 | |||
Suárez Mascareño et al. (2017) | act | 34.8 ± 1.3 | 21.8 ± 0.1 | 30.0 ± 0.9 | 26.3 ± 5.6 | 37.2 ± 6.7 | |
Díez Alonso et al. (2019) | phm | 33.8 ± 0.6 | 21.6 ± 0.2 | 14.6 ± 0.2 | 29.5 ± 0.1 | 39.5 ± 0.2 | |
Sabotta et al. (2021) | act | 37.08 | 10.65, 21.4 |
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