Table 2
Already-known bright red high proper-motion objects: dwarfs.
| TYC | α | δ | VT | J | H | Ks | μ | π | Spectral | Name | Ref.c |
| (J2000) | (J2000) | [mag] | [mag] | [mag] | [mag] | [mas a-1] | [mas] | type | |||
|
|
|||||||||||
| 5913–1376–1 | 05 06 49.48 | –21 35 03.7 | 11.71 ± 0.12 | 7.00 ± 0.02 | 6.39 ± 0.02 | 6.11 ± 0.02 | 53 ± 4 | 100:a | M3.5V+M4.5V | BD–21 1074 BC | 1,2,3 |
| 2944–1956–1 | 07 10 01.84 | +38 31 46.2 | 11.8 ± 0.2 | 6.73 ± 0.03 | 6.15 ± 0.05 | 5.85 ± 0.02 | 1043 ± 4 | 159 ± 3 | M4.5Ve SB2 | QY Aur AB | 4,5,6 |
| 183–2190–1 | 07 44 40.15 | +03 33 09.0 | 11.35 ± 0.12 | 6.58 ± 0.02 | 6.00 ± 0.04 | 5.698 ± 0.017 | 567 ± 2 | 168 ± 2 | M4.0V | YZ CMi AB | 7,8,9 |
| 2003–139–1 | 13 31 46.61 | +29 16 36.7 | 12.3 ± 0.2 | 7.56 ± 0.02 | 7.00 ± 0.02 | 6.72 ± 0.02 | 272 ± 3 | 80:b | M4.0V+M: | DG CVn AB | 10,11,12 |
Notes. (1) Stephenson (1986); (2) Reid et al. (2004); (3) Jao et al. (2003); (4) Ross (1939); (5) Pettersen (1975); (6) Tomkin & Pettersen (1986); (7) Ross (1937); (8) Raassen et al. (2007); (9) Kowalski et al. (2010); (10) Robb et al. (1999); (11) Beuzit et al. (2004); (12) Reiners & Basri (2010).
Photometric parallax from Reid et al. (1995).
Photometric parallax estimated from Beuzit et al. (2004).
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