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Table A.2.

Stellar and disk masses for the objects in the Chamaeleon I star-forming region.

2MASS name Other names Dist (pc) M M Mdisk,dust M
2MASSJ10533978-7712338 ... 191.81 0.33 2.2259 ± 1.7065
2MASSJ10555973-7724399 T3A 185.08 0.81 15.3631 ± 1.3908
2MASSJ10561638-7630530 ESOHalpha553 196.48 0.14 1.9879 ± 1.5696
2MASSJ10563044-7711393 T4 183.09 0.76 50.9436 ± 1.3219
2MASSJ10574219-7659356 T5 190.00 0.32 4.2586 ± 1.5444
2MASSJ10580597-7711501 ... 186.57 0.11 1.2118 ± 1.4433
2MASSJ10581677-7717170 T6 189.84 1.47 147.4129 ± 1.4123
2MASSJ10590108-7722407 T7 185.21 0.76 29.3149 ± 1.3753
2MASSJ10590699-7701404 T8 187.48 2.00 203.0813 ± 1.3752
2MASSJ11004022-7619280 T10 191.54 0.23 33.5953 ± 1.4367
2MASSJ11022491-7733357 T11 176.26 1.50 92.0593 ± 1.2175
2MASSJ11025504-7721508 T12 182.24 0.19 0.5047 ± 1.4892
2MASSJ11040425-7639328 CHSM1715 192.31 0.18 1.3482 ± 1.5306
2MASSJ11040909-7627193 T14 191.78 0.96 49.8157 ± 1.4450
2MASSJ11044258-7741571 ISO52 193.15 0.23 2.0116 ± 1.5144
2MASSJ11045701-7715569 T16 194.46 0.29 1.2572 ± 2.0343
2MASSJ11062554-7633418 ESOHalpha559 209.30 0.13 26.5032 ± 1.7167
2MASSJ11064180-7635489 Hn5 195.28 0.17 0.4820 ± 1.7566
2MASSJ11065906-7718535 T23 190.34 0.25 11.5032 ± 1.4359
2MASSJ11065939-7530559 ... 196.24 0.11 1.5752 ± 1.5836
2MASSJ11071206-7632232 T24 195.75 0.54 2.1143 ± 1.9855
2MASSJ11071860-7732516 ChaHalpha9 198.58 0.13 0.4760 ± 1.8295
2MASSJ11072074-7738073 T26 190.62 2.35 12.3622 ± 1.5004
2MASSJ11074245-7733593 ChaHalpha2 190.00 0.13 1.1201 ± 1.6764
2MASSJ11074366-7739411 T28 194.81 0.45 52.5996 ± 1.4903
2MASSJ11074656-7615174 CHSM10862 194.22 0.07 1.0675 ± 1.5858
2MASSJ11075730-7717262 CHXR30B 187.10 0.44 2.9235 ± 1.5474
2MASSJ11075792-7738449 T29 163.19 1.01 6.8730 ± 1.1208
2MASSJ11075809-7742413 T30 184.46 0.29 2.8416 ± 1.5023
2MASSJ11080148-7742288 T31 190.00 0.75 20.8577 ± 1.4490
2MASSJ11080297-7738425 ISO126 190.00 0.53 47.7823 ± 1.4183
2MASSJ11081509-7733531 T33A 190.00 1.40 97.5590 ± 1.4131
2MASSJ11083905-7716042 T35 188.36 0.78 6.4824 ± 1.5029
2MASSJ11085367-7521359 ... 188.27 0.49 11.5165 ± 1.4639
2MASSJ11085464-7702129 T38 186.01 0.60 1.7817 ± 1.6551
2MASSJ11092266-7634320 C1-6 203.25 0.56 2.0788 ± 1.9762
2MASSJ11092379-7623207 T40 192.31 0.48 58.8523 ± 1.4513
2MASSJ11094621-7634463 Hn10E 195.04 0.33 2.3551 ± 1.7559
2MASSJ11094742-7726290 B43 192.96 0.53 71.2352 ± 1.4628
2MASSJ11095340-7634255 T42 201.96 0.72 40.9535 ± 1.6319
2MASSJ11095407-7629253 T43 190.00 0.52 14.4300 ± 1.4688
2MASSJ11095873-7737088 T45 191.29 0.47 9.8888 ± 1.4691
2MASSJ11100010-7634578 T44 192.08 1.90 658.7556 ± 1.4422
2MASSJ11100369-7633291 Hn11 201.01 0.59 5.2263 ± 1.7104
2MASSJ11100469-7635452 T45A 195.01 0.76 3.8183 ± 1.6431
2MASSJ11100704-7629376 T46 179.61 0.72 3.0229 ± 1.4048
2MASSJ11101141-7635292 ISO237 195.37 1.02 36.5996 ± 1.5194
2MASSJ11103801-7732399 CHXR47 190.00 1.30 2.5077 ± 1.6307
2MASSJ11104959-7717517 T47 185.16 0.38 26.1129 ± 1.3729
2MASSJ11105333-7634319 T48 194.68 0.29 15.1497 ± 1.5435
2MASSJ11105359-7725004 ISO256 195.77 0.16 3.9378 ± 1.5630
2MASSJ11105597-7645325 Hn13 140.23 0.12 0.5694 ± 0.8777
2MASSJ11111083-7641574 ESOHalpha569 190.00 . . . 25.6606 ± 1.4564
2MASSJ11113965-7620152 T49 190.51 0.25 10.2706 ± 1.4716
2MASSJ11114632-7620092 CHX18N 192.51 1.40 17.0085 ± 1.5003
2MASSJ11120351-7726009 ISO282 185.49 0.14 1.3134 ± 1.4191
2MASSJ11120984-7634366 T50 193.23 0.18 2.1573 ± 1.5650
2MASSJ11122772-7644223 T52 193.24 1.87 28.4416 ± 1.4909
2MASSJ11123092-7644241 T53 196.00 0.56 6.1133 ± 1.6065
2MASSJ11132446-7629227 Hn18 189.52 0.23 3.7763 ± 1.5473
2MASSJ11142454-7733062 Hn21W 188.95 0.19 3.5031 ± 1.4600
2MASSJ11160287-7624533 ESOHalpha574 190.00 . . . 6.0154 ± 1.6076
2MASSJ11173700-7704381 T56 188.38 0.49 12.9369 ± 1.4509
2MASSJ11183572-7935548 . . . 94.62 0.17 1.7129 ± 0.3583
2MASSJ11241186-7630425 . . . 184.75 0.13 0.6530 ± 1.4867
2MASSJ11432669-7804454 . . . 180.63 0.14 0.5826 ± 1.8409

Notes. Original stellar masses are from Manara et al. (2016a, 2017). Original disk masses are from Pascucci et al. (2016). The distances used to modify these values are from Gaia Collaboration (2018).

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