Table 1
Source properties taken from the literature.
| Name | D | Sep. | Memb. | Sp. type | A v | T eff b | log gb | L bol | Mass | References |
| (pc) | (′′) | (mag) | (K) | (dex) | (dex ) | (MJup) | ||||
|
|
||||||||||
| Cha1109 | ~165 | – | Cha I | M9.5 ± 0.5a | 1 ± 1 | – | – | –3.33 | 8 |
1,2,41 |
| AB Pic b | 45.5 | 5.5 | Tuc-Hor | L0–L1 | 0.27 ± 0.02 | 2000 |
4.0 ± 0.5 | –3.6 ± 0.2 | 10–14 | 3, 4, 6, 7 |
| Carina | 5 | |||||||||
| DH Tau B | ~140 | 2.3 | Taurus | – | 2.7–2.8 | 2700-2800 | 4.0–4.5 | ~–2.44 | 30–50 | 8 |
| 142 | 1.1 ± 1.1 | –2.71 ± 0.12 | 11 |
9 | ||||||
| GSC08047 B | 85–92 | 3.3 | Tuc-Hor | M9.5 ± 1 | – | – | – | –3.3 ± 0.1 | 25 ± 10 | 5, 10, 11, 12, 46 |
| TWA 22A | 17.5 | 0.09 | β Pic | M6 ± 1 | – | 2900 ± 200 | 4.0–5.5 | –2.11 ± 0.13 | 220 ± 21c | 13, 14, 46 |
| TWA 22B | 17.5 | 0.09 | β Pic | M6 ± 1 | – | 2900 |
4.0–5.5 | –2.30 ± 0.16 | 220 ± 21c | 13, 14, 46 |
| 2M1207 A | 52.4 | – | TWA | M8.25 ± 0.50a | ~0.0 | 2550 ± 150 | 4.0 ± 0.5 | –2.72 | 24 ± 6 | 15, 16, 17, 18 |
| OTS44 | ~165 | – | Cha I | M9.5 ± 1a | 0.0 | – | – | –3.11 | ~15 | 2, 19, 20 |
| KPNO 4 | ~140 | – | Taurus | M9.5 a |
0.0 | – | – | –2.64 | ~15 | 20, 21, 22 |
| 4 | –2.0 | 10 | 23 | |||||||
| 2.45 | 24 | |||||||||
| 2M0141 | ~41 | – | Field | L0a | – | 2000 ± 100 | 4.0 ± 0.5 | –3.5 | 12 |
25,26 |
| TWA 5B | 50 | 1.96 | TWA | M8.5–M9a | – | 2750 ± 200 | 3.9 ± 0.6 | –2.68 ± 0.07 | 20–25 | 27, 28, 29, 47 |
| Gl 417 Bd | 21.7 | ~92 | Field | L4.5a | – | 1800–1900 | 5.5–6.0 | – | 35 ± 15 | 30, 31, 32, 33 |
| 2M0345 | 26.9 | – | UMa | L0a | – | 2000 | 6 | –3.60 | – | 34, 35, 36, 38, 39 |
| 1900 | 5.5 | 37 | ||||||||
| 2200 | 5.0 | 40 | ||||||||
| CT Cha b | ~165 | 2.67 | Cha I | M8-L0 | 5.2 ± 0.8 | 2600 ± 250 | 3.5 | −2.68 ± 0.21 | 8–23 | 42 |
| USco 108 B | 145 | 4.6 | USco | M9.5a | – | – | – | −3.14 ± 0.20 |
|
43 |
| HR7329 B | 48.2 | 4.2 | β Pic | M7-M8a | – | – | – | −2.63 ± 0.09 | 20–50 | 44, 45 |
Notes.
Bouy et al. (2003) resolved the companion Gl 417 B as a tight binary. Kirkpatrick et al. (2008) classified this object L4.5pec in the optical and suggest it is composed of a pair of L4 + L6/L6.5 or L4.5 + L6.5/L7 brown dwarfs using a relation between MI and spectral types.
Reference. (1) Luhman et al. (2005a); (2) Luhman (2007); (3) Song et al. (2003); (4) van Belle et al. (2009); (5) Torres et al. (2008); (6) Bonnefoy et al. (2010); (7) Chauvin et al. (2005b); (8) Itoh et al. (2005); (9) Luhman et al. (2006); (10) Chauvin et al. (2003); (11) Chauvin et al. (2005a); (12) Neuhäuser & Guenther (2004); (13) Bonnefoy et al. (2009); (14) Teixeira et al. (2009); (15) Gizis (2002); (16) Herczeg et al. (2009); (17) Ducourant et al. (2008); (18) Mohanty et al. (2007); (19) Tamura et al. (1998); (20) Luhman et al. (2004); (21) Briceño et al. (2002); (22) McGovern et al. (2004); (23) Kraus et al. (2006); (24) Guieu et al. (2007); (25) Kirkpatrick et al. (2006); (26) Cruz et al. (2009); (27) Lowrance et al. (1999); (28) Neuhäuser et al. (2000); (29) Rice et al. (2010); (30) Kirkpatrick et al. (2000); (31) Kirkpatrick et al. (2001); (32) Kirkpatrick et al. (2008); (33) Testi (2009); (34) Kirkpatrick et al. (1997); (35) Kirkpatrick et al. (1999); (36) Leggett et al. (2001); (37) Schweitzer et al. (2001); (38) Dahn et al. (2002); (39) Bannister & Jameson (2007); (40) Lyubchik et al. (2007); (41) Luhman et al. (2008); (42) Schmidt et al. (2008); (43) Béjar et al. (2008); (44) Lowrance et al. (2000); (45) Neuhäuser et al. (2011); (46) Malo et al. (2013); (47) Weinberger et al. (2013).
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