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Table 11

Previous kinematical results based on studies of nearby late-type dwarfs.

Study Stellar Sample σ U σ V σ W V a v Comments on sample selection
sample size (km s-1) (km s-1) (km s-1) (km s-1) (°)

Wielen (1977) All stars 516 39 23 20 MCC stars with HK data
~ 0.3 Gyr 18 10 8 MCC stars with HK +8/+3
~5 Gyr 38 23 20 MCC stars with HK 0
~9 Gyr 66 27 23 MCC stars with HK –2/5
Reid et al. (1995) M-type 368 39 26 23 MCC M dwarfs in PMSU I survey
Reid et al. (1995) Hα 86 27 23 21 CNS3 M dwarfs with Hα emission
Reid et al. (1995) M-type 514 43 31 25 CNS3 M dwarfs within 25 pc
Ratnatunga & Upgren (1997) Young disk 30.6 18.5 12.4 –7.4 11.7 MCC stars (max. likelihood),
Old disk 54.0 35.9 31.3 –23.0 with pre-Hipparcos astrometry
Upgren et al. (1997) Young disk 30.2 17.3 11.9 –8.2 9.7 MCC stars (max. likelihood),
Old disk 56.1 34.2 31.2 –28.3 with post-Hipparcos astrometry
Reid et al. (2002) dMe 83 25.0 21.1 17.8 CNS3 dMe in PMSU IV survey
dM+dMe 436 37.9 26.1 20.5 CNS3 dM+dMe in PMSU IV
Bochanski et al. (2005) Active 155 19 15 16 M dwarfs within 100 pc
Bochanski et al. (2005) Inactive 419 35 21 22 M dwarfs within 100 pc
Bochanski et al. (2007) M-type 70 28.4 21.3 19.2 SDSS M dwarfs, | z | < 100 pc
Fuchs et al. (2009) M-type 48 075 32.4 23.0 18.1 SDSS M dwarfs, | z | < 100 pc

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