Table F.1
Literature properties of the sample.
No. | Main | Alternative | Region | d | Teff | AV | Multiplicity | F1.3mm | Reference |
---|---|---|---|---|---|---|---|---|---|
name | name | (pc) | (K) | (mag) | (mJy) | ||||
1 | HD31293 | AB Aur | Taurus | 162.9 ± 1.6 | 9800 | 0.2 | (*) | 136±15 | b,1 |
2 | HD31648 | MWC480 | Taurus | 161.8 ± 2.1 | 8800 | 0.2 | (*) | 250±15 | b,1 |
3 | HD34282 | Ori A | 311.5 ± 4.9 | 9400 | 0.6 | (*) | 100±23 | a,2 | |
4 | HD36112 | MWC758 | Taurus | 160.3 ± 1.8 | 8200 | 0.2 | (*) | 72±13 | b,3 |
5 | HD97048 | CU Cha | Chamaeleon | 184.8 ± 1.4 | 10400 | 1.1 | (*) | 452±34 | a,4 |
6 | HD100453 | Lower Cen | 104.2 ± 0.4 | 7200 | 0.0 | (*)* | 200±21 | a,5 | |
7 | HD100546 | Lower Cen | 110.0 ± 0.6 | 9800 | 0.1 | (*) | 465±20 | a,4 | |
8 | HD135344B | SAO 206462 | Upper Cen | 135.7 ± 1.5 | 6400 | 0.4 | (*) | 142±19 | a,6 |
9 | HD139614 | Upper Cen | 134.8 ± 0.9 | 7800 | 0.0 | (*) | 242±15 | a,6 | |
10 | HD142527 | Upper Cen | 157.2 ±1.2 | 6400 | 0.6 | (**) | 1190±33 | a,7 | |
11 | HD142666 | Upper Sco | 148.4 ± 1.1 | 7400 | 0.9 | (*) | 127±9 | a,6 | |
12 | HD143006 | J1558.3-2257 | Upper Sco | 166.1 ± 4.2 | 5800 | 0.7 | (*) | 43 ± 3(1.2) | g,2 |
13 | HD144432 | Upper Sco | 155.3 ± 1.5 | 7400 | 0.4 | (*)* | 44±10 | a,7 | |
14 | HD144668 | HR5999 | Lupus | 161.0 ± 1.8 | 8400 | 0.5 | (*)* | 20±16 | a,4 |
15 | HD145718 | V718 Sco | Upper Sco | 152.4 ± 1.9 | 8000 | 0.5 | (*) | 49±5 | a,29 |
16 | HD150193A | Upper Sco | 150.8 ± 1.6 | 9000 | 1.5 | (*)* | 45±12 | a,1 | |
17 | HD152404 | AK Sco | Upper Sco | 140.6 ± 1.2 | 6200 | 0.7 | (**) | 33±1 | a,8 |
18 | HD163296 | Upper Sco | 101.5 ± 1.1 | 9200 | 0.5 | (*) | 743±15 | a,4 | |
19 | HD169142 | - | 114.0 ± 0.8 | 7400 | 0.0 | (*) | 197±15 | b,6 | |
20 | HD179218 | - | 266.0 ± 3.6 | 9600 | 0.4 | (*)* | 71±7 | b,3 | |
21 | TW Hya | - | 60.1 ± 0.1 | 4000 | 0.0 | (*) | 558±1 | d,9 | |
22 | PDS 70 | V1032 Cen | Upper Cen | 113.4 ± 0.5 | 4000 | 0.0 | (*) | 233 ± 3(0.87) | i,18 |
23 | RX J1604.3-2130 | Upper Sco | 150.2 ± 1.4 | 4600 | 1.1 | (*) | 69±1 | h,10 | |
24 | EM* SR21 | Rho Oph | 138.3 ± 1.2 | 5800 | 6.3 | (*) | 95±10 | d, 21 | |
25 | GG Tau A | Taurus | 150.2 ± 2.3 | 4000 | 0.3 | (***) | 593±53 | f,12 | |
26 | Sz 91 | Lupus | 159.0 ± 1.5 | 3800 | 1.9 | (*) | <27 | c,25 | |
27 | DoAr 28 | V2251 Oph | Rho Oph | 138.9 ± 1.0 | 4400 | 1.9 | (*) | <75 | j,11 |
28 | LkCa15 | Taurus | 159.0 ± 1.3 | 4800 | 0.6 | (*) | 167±6 | d,14 | |
29 | WLY 2-48 | Oph IRS 48 | Rho Oph | 134.4 ± 2.2 | 9000 | 10.0 | (*) | 60±10 | g,11 |
30 | V4046 Sgr | - | 72.4 ± 0.3 | 4000 | 0.0 | (**) | 283±28 | k,15 | |
31 | PDS 66 | MP Mus | - | 98.9 ± 0.3 | 4600 | 0.8 | (*) | 224±8 | l,16 |
32 | LkHα330 | Perseus | 310.6 ± 7.9 | 5800 | 3.0 | (*) | 53±2 | d,17 | |
33 | GM Aur | Taurus | 159.7 ± 2.1 | 4400 | 1.4 | (*) | 253±12 | d,12 | |
34 | RX J1615.3-3255 | Lupus | 157.7 ± 1.0 | 4000 | 0.6 | (*) | 132±4 | d,16 | |
35 | V1247 Ori | HD290764 | Ori OB1 | 398.4 ± 9.8 | 7800 | 0.3 | (*) | 174 ± 23(0.87) | a,24 |
36 | T Cha | Chamaeleon | 109.6 ± 1.0 | 5200 | 1.2 | (*) | 105±15 | l,16 | |
37 | DoAr 44 | Rho Oph | 146.0 ± 1.1 | 4800 | 2.2 | (*) | 105±11 | d,19 | |
38 | DZ Cha | Chamaeleon | 100.8 ± 0.3 | 3600 | 0.2 | (*) | <24(0.87) | l,20 | |
39 | AS209 | Upper Sco | 120.9 ± 0.9 | 4400 | 0.8 | (*) | 300±30 | g,21 | |
40 | IM Lup | Lupus | 158.5 ± 1.3 | 4400 | 0.5 | (*) | 260±9 | c,25 | |
41 | MY Lup | Lupus | 156.5 ± 1.2 | 5000 | 1.2 | (*) | 56±4 | c,23 | |
42 | RU Lup | Lupus | 159.5 ± 1.8 | 4000 | 0.0 | (*) | 197±7 | c,25 | |
43 | RY Lup | Lupus | 159.0 ± 1.8 | 4800 | 2.0 | (*) | 78±5 | c,23 | |
44 | CI Tau | Taurus | 158.7 ± 1.3 | 4400 | 1.9 | (*) | 190±17 | f,12 | |
45 | CQ Tau | HD36910 | Taurus | 163.1 ± 2.2 | 6800 | 0.4 | (*) | 172±1 | m,10 |
46 | CS Cha | Chamaeleon | 176.4 ± 1.3 | 4800 | 0.6 | (**)* | 129±46 | d,4 | |
47 | CV Cha | Chamaeleon | 193.4 ± 1.1 | 5200 | 1.5 | (*) | 59 ± 1(0.88) | e,28 | |
48 | IRAS 16051-3820 | J1608-3828 | Lupus | 156.0 ± 1.0 | 4800 | 0.0 | (*) | 39±1 | c,22 |
49 | Sz 111 | Lupus | 158.2 ± 0.8 | 3800 | 0.0 | (*) | 49±5 | c,16 | |
50 | UX Tau A | Taurus | 139.9 ± 2.0 | 5000 | 1.2 | (*)* | 65±1 | f,10 | |
51 | DI Cha | Sz 19 | Chamaeleon | 190.5 ± 1.1 | 5200 | 1.8 | (*)* | 38±11 | e,4 |
52 | IRAS 08267-3336 | AT Pyx | Gum Nebula | 373.1 ± 7.1 | 5000 | 1.2 | (*) | f | |
53 | SY Cha | J1056.3-7711 | Chamaeleon | 183.2 ± 0.7 | 4000 | 0.6 | (*) | 118 ± 1(0.88) | e,28 |
54 | VZ Cha | Chamaeleon | 192.3 ± 0.7 | 3800 | 2.0 | (*) | 123 ± 1(0.88) | e,27 | |
55 | EX Lup | Lupus | 157.7 ± 1.0 | 3800 | 0.0 | (*) | 19±4 | c,23 | |
56 | RX J1852.3 | CrA | 145.8 ± 1.1 | 4800 | 0.3 | (*) | 60±8 | d,26 | |
57 | Sz 71 | GW Lup | Lupus | 156.0 ± 1.5 | 3600 | 0.8 | (*) | 106±18 | c,25 |
58 | SZ Cha | Chamaeleon | 189.8 ± 1.5 | 4900 | 1.5 | (*) | 78 ± 20(1.2) | d,13 |
Notes. Columns are: reference number in this work; main name; alternative name from the literature; star forming region; distance from Gaia DR2 (Gaia Collaboration 2018); effective temperature and optical extinction adopted in this work; stellar multiplicity, with star(s) indicated by asterisks and the disk by the brackets; flux at 1.3 mm, unless differently specified by the superscript number; reference for the effective temperature (letters) and millimeter flux (numbers), as specified below.
References. a. Fairlamb et al. (2015), b. Folsom et al. (2012), c. Alcalá et al. (2017), d. Manara et al. (2014), e. Manara et al. (2017), f. Herczeg & Hillenbrand (2014), g. Salyk et al. (2013), h. Preibisch & Zinnecker (1999), i. Kunder et al. (2017), j. Rich et al. (2015), k. Pecaut & Mamajek (2013), l. da Silva et al. (2009), m. Pascual et al. (2016). 1. Sandell et al. (2011), 2. Natta et al. (2004), 3. Mannings & Sargent (2000), 4. Henning et al. (1994), 5. Meeus et al. (2002), 6. Sylvester et al. (1996), 7. Walker & Butner (1995), 8. Czekala et al. (2015), 9. Tsukagoshi et al. (2016), 10. Pinilla et al. (2018), 11. Andrews & Williams (2007), 12. Beckwith et al. (1990), 13. Ubach et al. (2012), 14. Osterloh & Beckwith (1995), 15. Rosenfeld et al. (2013), 16. van der Marel et al. (2016), 17. Isella et al. (2013), 18. Long et al. (2018), 19. Nuernberger et al. (1998), 20. Canovas et al. (2018), 21. Andre & Montmerle (1994), 22. Ansdell et al. (2018), 23. Lommen et al. (2010), 24. Kraus et al. (2017), 25. Nuernberger et al. (1997), 26. Hughes et al. (2010), 27. Long et al. (2017), 28. Andrews et al. (2013), 29. ALMA archive.
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