Table 1
Source properties.
Name | RA (J2000) | Dec (J2000) | F 890 μm | rms | d | M ⋆ | L ⋆ | SpT | T eff |
(mJy) | (mJy/beam) | (pc) | (M⊙) | (L⊙) | (K) | ||||
|
|||||||||
Sz 65 | 15:39:27.75 | –34:46:17.56 | 64.49 | 0.32 | 150 | 0.76 | 0.832 | K7 | 4060 |
J15450887-3417333 | 15:45:08.85 | –34:17:33.81 | 46.27 | 0.5 | 150 | 0.14 | 0.058 | M5.5 | 3060 |
Sz 68 | 15:45:12.84 | –34:17:30.98 | 150.37 | 0.46 | 150 | 2.13 | 5.129 | K2 | 4900 |
Sz 69 | 15:45:17.39 | –34:18:28.66 | 16.96 | 0.28 | 150 | 0.19 | 0.088 | M4.5 | 3197 |
Sz 71 | 15:46:44.71 | –34:30:36.05 | 166.04 | 0.63 | 150 | 0.42 | 0.309 | M1.5 | 3632 |
Sz 73 | 15:47:56.92 | –35:14:35.15 | 30.43 | 0.55 | 150 | 0.82 | 0.419 | K7 | 4060 |
IM Lup | 15:56:09.18 | –37:56:06.12 | 600.0 | 0.13 | 150 | 1.0 | 1.65 | M0 | 3850 |
Sz 83 | 15:56:42.29 | –37:49:15.82 | 426.9 | 0.72 | 150 | 0.75 | 1.313 | K7 | 4060 |
Sz 84 | 15:58:02.50 | –37:36:03.08 | 32.64 | 0.4 | 150 | 0.18 | 0.122 | M5.0 | 3125 |
Sz 129 | 15:59:16.45 | –41:57:10.66 | 181.12 | 0.52 | 150 | 0.8 | 0.372 | K7 | 4060 |
J16000236–4222145 | 16:00:02.34 | –42:22:14.99 | 119.85 | 0.63 | 150 | 0.24 | 0.148 | M4 | 3270 |
MY Lup | 16:00:44.50 | –41:55:31.27 | 176.81 | 0.76 | 150 | 1.02 | 0.776 | K0 | 5100 |
Sz 133 | 16:03:29.37 | –41:40:02.14 | 69.05 | 0.77 | 150 | 0.63 | 0.07 | K2 | 4900 |
Sz 90 | 16:07:10.05 | –39:11:03.64 | 21.83 | 0.46 | 200 | 0.79 | 0.661 | K7 | 4060 |
Sz 98 | 16:08:22.48 | –39:04:46.81 | 237.29 | 1.42 | 200 | 0.74 | 2.512 | K7 | 4060 |
Sz 100 | 16:08:25.74 | –39:06:1.63 | 54.85 | 0.58 | 200 | 0.18 | 0.169 | M5.5 | 3057 |
Sz 108B | 16:08:42.86 | –39:06:15.04 | 26.77 | 0.34 | 200 | 0.19 | 0.151 | M5 | 3125 |
J16085324–3914401 | 16:08:53.22 | –39:14:40.53 | 19.57 | 0.28 | 200 | 0.32 | 0.302 | M3 | 3415 |
Sz 113 | 16:08:57.78 | –39:02:23.21 | 22.35 | 0.27 | 200 | 0.19 | 0.064 | M4.5 | 3197 |
Sz 114 | 16:09:01.83 | –39:05:12.79 | 96.41 | 0.41 | 200 | 0.23 | 0.312 | M4.8 | 3175 |
J16102955–3922144 | 16:10:29.53 | –39:22:14.83 | 7.14 | 0.35 | 200 | 0.22 | 0.158 | M4.5 | 3200 |
J16124373–3815031 | 16:12:43.73 | –38:15:03.40 | 29.88 | 0.49 | 200 | 0.47 | 0.617 | M1 | 3705 |
Notes. F890 μm is the integrated flux and rms is the root mean square noise from Ansdell et al. (2016). d is the distance to the source: for sources in the Lupus I, II and IV clouds d = 150 pc, while for stars in the Lupus III cloud d = 200 pc (see Comerón 2008). We note that recent measurements from the Gaia space telescope might suggest a distance of 150 pc for the Lupus III cloud. M⋆ is the stellar mass as in Ansdell et al. (2016), obtained using evolutionary tracks by Siess et al. (2000). Stellar bolometric luminosity L⋆, effective temperature Teff and spectral type SpT are derived from X-shooter measurements by (Alcalá et al. 2014, 2017).
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