Table 1
Sample parameters.
No. | 2MASS ID | Cloud | Distance | Spectral type | Hα width | Ref. | Binary sep. | Binary ref. | |
(parsecs) | (km s-1) | (arsecs) | |||||||
|
|||||||||
1 | 04182147+1658470 | Taurus | 135 ± 20 | K5 | Absorp. | 1, 2, 3 | ... | ... | |
2 | 04192625+2826142 | Taurus | 135 ± 20 | K7 | 180 | 4, 5 | 10.5 | 1 | |
3 | 04242321+2650084 | Taurus | 135 ± 20 | M2 | 200 | 5 | ... | ... | |
4 | 04314503+2859081 | Taurus | 135 ± 20 | F5 | Absorp. | 5 | ... | ... | |
5 | 04325323+1735337 | Taurus | 135 ± 20 | M2 | 138 | 4, 6 | ... | ... | |
6 | 04330422+2921499 | Taurus | 135 ± 20 | B9 | Absorp. | 5 | ... | ... | |
7 | 04364912+2412588 | Taurus | 135 ± 20 | F2 | Absorp. | 2, 5 | ... | ... | |
8 | 04403979+2519061 | Taurus | 135 ± 20 | M5 | 130 | 3, 5 | ... | ... | |
9 | 04420548+2522562 | Taurus | 135 ± 20 | K7 | 94 | 3, 6 | 0.3 | 11 | |
10 | 08413703-7903304 | η Chamaleonis | 97 ± 3 | M3 | Absorp. | 4, 7 | ... | ... | |
11 | 08422372-7904030 | η Chamaleonis | 97 ± 3 | M3 | Absorp. | 4, 7 | ... | ... | |
12 | 11073519-7734493 | Chamaleon I | 160 ± 15 | M4 | 89 | 1, 8 | ... | ... | |
13 | 11124268-7722230 | Chamaleon I | 160 ± 15 | G8 | Absorp. | 1, 8, 9 | 0.247 | 12 | |
14 | 16002612-4153553 | Lupus IV | 150 ± 20 | M5.25 | 162 | 10 | 2.8 | 13 | |
15 | 16010896-3320141 | Lupus I | 150 ± 20 | G8 | Absorp. | 6 | ... | ... | |
16 | 16031181-3239202 | Lupus I | 150 ± 20 | K7 | 132 | 4, 6 | ... | ... | |
17 | 16085553-3902339 | Lup III | 200 ± 20 | M6 | 189 | 10 | 2.8 | 13 | |
18 | 16124119-1924182 | Ophiuchus | 119 ± 6 | K8 | 131 | 6 | 1.0 | 14 | |
19 | 16220961-1953005 | Ophiuchus | 119 ± 6 | M3.7 | 132 | 10 | 1.8,3 | 10 | |
20 | 16223757-2345508 | Ophiuchus | 119 ± 6 | M2.5 | 128 | 4, 6 | ... | ... | |
21 | 16251469-2456069 | Ophiuchus | 119 ± 6 | M0 | 206 | 4, 6 | ... | ... | |
22 | 16275209-2440503 | Ophiuchus | 119 ± 6 | K7 | 151 | 4 | 0.480 | 15 | |
23 | 19002906-3656036 | Corona Australis | 129 ± 11 | M4 | 93 | 10 | 0.132 | 16 | |
24 | 19012901-3701484 | Corona Australis | 129 ± 11 | M3.75 | 83 | 10 | 0.5 | 10 |
Reference. The target’s photometry, spectral types and Hα widths can be found in the following papers. 1) Nguyen et al. (2012); 2) Howard et al. (2013); 3) Luhman et al. (2010); 4) Cieza et al. (2013); 5) Cieza et al. (2012); 6) Wahhaj et al. (2010); 7) Sicilia-Aguilar et al. (2009); 8) Luhman et al. (2008); 9) Matrà et al. (2012); 10) Romero et al. (2012). The binary systems were identified in the following papers: 11) Leinert et al. (1993); 12) Lafrenière et al. (2008); 13) Merín et al. (2008); 14) Prato (2007); 15) Ratzka et al. (2005); 16) Köhler et al. (2008).
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