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Table 1

JOYS source sample and physical properties.

Source RAa Deca d Lbol Tbol Class Menv Binary Other names Ref.
[J2000] [J2000] (pc) (L) (K) (M)
IRAS4B 03:29:12.02 +31:13:08.0 293 6.8 28 0 4.7 10.7 Per-emb 13 1-5
IRAS4A1b 03:29:10.54 +31:13:30.9 293 14.1 34 0 8.7 1.8 Per-emb 12 1-5
IRAS4A2b 03:29:10.43 +31:13:32.1 293 14.1 34 0 8.7 1.8 Per-emb 12 1-5
B1-c 03:33:17.88 +31:09:31.8 293 5.0 48 0 5.3 Per-emb 29 1-5
B1-b 03:33:20.34 +31:07:21.4 293 0.23 157 I 2.1 14 Per-emb 41 1,2,5
B1-a-1 03:33:16.67 +31:07:54.9 293 2.3 113 I 1.5 0.4 Per-emb 40 1-3, 5
B1-a-2 03:33:16.68 +31:07:55.3 293 2.3 113 I 1.5 0.4 Per-emb 40 1-3, 5
L1448-mm 03:25:38.88 +30:44:05.3 293 8.5 49 0 3.9 8.1 Per-emb 26 1-5
Per-emb 8 03:44:43.98 +32:01:35.2 321 4.5 45 0 1.0 9.6 - 1-5
TMC1-W 04:41:12.69 +25:46:34.7 142 0.7 161 I 0.2 0.6 IRAS 04381+2540 3 ,4, 6, 7
TMC1-E 04:41:12.73 +25:46:34.8 142 0.7 161 I 0.2 0.6 IRAS 04381+2540 3, 4, 6, 7
TMC1A 04:39:35.20 +25:41:44.2 142 2.7 189 I 0.2 - IRAS 04365+2535 3, 4, 6,7
L1527 IRS 04:39:53.88 +26:03:09.5 142 3.1 79 I 0.9 IRAS 04368+2557 3, 4, 6, 7
BHR71 IRS1 12:01:36.50 -65:08:49.4 200 14.7 68 0 19 15.7 IRAS 11590–6452 8-11
BHR71 IRS2 12:01:34.01 -65:08:48.0 200 1.7 38 0 19 15.7 - 8-11
Ser-SMM1-a 18:29:49.81 +1:15:20.4 436 109 39 0 58 2.0 Ser-emb 6 2, 3, 4, 12, 13
Ser-SMM1-b1 18:29:49.68 +1:15:21.1 436 109 39 0 58 0.3 - 2, 3, 4, 12, 13
Ser-SMM1-b2 18:29:49.66 +1:15:21.2 436 109 39 0 58 0.3 - 2,3,4,12,13
Ser-SMM3 18:29:59.31 +1:14:00.3 436 27.5 37 0 11.5 2, 3, 4, 14
Ser-S68N-N 18:29:48.13 +1:16:44.6 436 >6.0 58 0 10.4 1.4 - 2, 5, 15, 16
Ser-S68N-S 18:29:48.09 +1:16:43.3 436 >6.0 58 0 10.4 1.4 Ser-emb 8 2, 5, 15, 16
Ser-emb-8(N)b 18:29:48.73 +1:16:55.6 436 1.8 0 6.6 SerpM-S68Nb 2, 15, 17, 18, 19
HH 211 03:43:56.81 +32:00:50.2 321 4.1 27 0 2.4 - Per-emb 1 1, 2, 25
G28IRS2 18:42:51.99 -3:59:54.0 4510 10120 IRDC/ 3288 G28P2 22, 23
- HMPO
G28P1 18:42:50.59 -4:03:16.3 4510 682 IRDC 4276 22, 23
G28S 18:42:46.45 -4:04:15.2 4510 364 IRDC 2296 22, 23
IRAS 23385 23:40:54.49 +61:10:27.4 4900 3170 - HMPO 220 - Mol160 20, 21
IRAS 18089 18:11:51.24 -17:31:30.4 2340 15 723* HMC 1100* G12.89+0.49 23, 24
G31 18:47:34.33 -1:12:45.5 5160 69 984 HMC 7889 22, 23

Notes. 1- Tobin et al. (2016), 2- Ortiz-León et al. (2018) , 3- Karska et al. (2018), 4- Kristensen et al. (2012), 5- Enoch et al. (2009), 6- Krolikowski et al. (2021), 7- van’t Hoff et al. (2020), 8- Yang et al. (2020), 9- Seidensticker & Schmidt-Kaler (1989), 10- Tobin et al. (2019), 11- Yang et al. (2017), 12- Hull et al. (2017), 13- ALMA 2015.1.00354.S, 14- 2017.1.01350.S, 15- Le Gouellec et al. (2019), 16 - 2015.1.00768.S, 17- Tychoniec et al. (2021), 18- Podio et al. (2021), 19- 2019.1.00931.S, 20- Beuther et al. (2023), 21- Molinari et al. (2008), 22- Wang et al. (2008), 23- Urquhart et al. (2018), 24- Xu et al. (2011), 25- Sadavoy et al. (2014). *Distance corrected. Properties scalable with distance are corrected according to updated distance measurement. a Coordinates of millimeter interferometry source position; MIRI IFU pointing is usually offset from source toward blue outflow lobe, see Table A.1 for IFU pointings. b Source continuum center not covered in MIRI 1290 observations.

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