Table A.1
Observational characteristics of FU Orionis objects.
| Object | Lobs | tbst | trise | Distance | Period of | Ref. |
|---|---|---|---|---|---|---|
| [L⊙] | [yr] | [yr] | [pc] | observ. | ||
| RNO1B/RNO1C | 1600 (†) | >100 | 0–12 | 930 | 2006–2010 | 1,2,3 |
| SVS13A | 25 | >30 | 2 | 235 | – | 4 |
| Gaia 17bpi | 7.5 | >4 | 1 | 1270 | – | 7 |
| V2775 Ori | 29 | 11–21 | 0–10 | 428 | 2006–2010 | 3,8 |
| FU Ori | 320 | >84 | 1 | 416 | 2004 | 9,10 |
| V900 Mon | 184 | >22 | 1–2 | 1500 | 2006–2010 | 3 |
| V960 Mon | 106 | 6 | 1 | 1638 | 2006–2010 | 3,13 |
| V1515 Cyg | 180 | >70 | 10 | 1009 | 2004 | 9,10 |
| HBC722 | 20 | >10 | <0.2 | 771 | 2016 | 14,15 |
| V1057 Cyg | 400 | 30–40 | 1 | 920 | 2004 | 9,10 |
| V2494 Cyg | 129 | >31 | 0–6 | 498 | 2006–2010 | 3,16 |
| V2495 Cyg | 21 | >19 | 0–1 | 600 | 2006–2010 | 3,17 |
| V1735 Cyg | 72 | 60 | 0–8 | 624 | 2006–2010 | 3,18 |
| V733 Cep | 30 | >67 | 0–18 | 669 | 2006–2020 | 18-20 |
| PP13S | 51 | >100 | – | 450 | 2006–2010 | 3,5 |
| L1551 IRS5 | 29 (†) | >100 | – | 147 | 2006–2010 | 3,6 |
| Haro 5a/6a IRS | 18 (†) | >100 | – | 388 | 2006–2010 | 3 |
| V883 Ori | 103 | >100 | – | 388 | 2006–2010 | 3 |
| NGC2071 MM3 | 35 | >100 | – | 388 | 2006–2010 | 3 |
| AR 6A/6B | 310 (†) | >100 | – | 738 | 2006–2010 | 3 |
| Parsamian 21 | 16 | >100 | – | 500 | 2006–2010 | 3 |
| BBW 76 | 106 | >120 | – | 1093 | 2004 | 10,11 |
References. 1 = Staude & Neckel (1991), 2 = Reid et al. (2014), 3 = Connelley & Reipurth (2018), 4 = De Simone et al. (2017), 5 = Lada et al. (2009), 6 = Loinard et al. (2007), 7 = Hillenbrand et al. (2018), 8 = Caratti o Garatti et al. (2011), 9 = Herbig (1977), 10 = Green et al. (2006), 11 = Ninan et al. (2013), 12 = Reipurth et al. (2012), 13 = Hackstein et al. (2015), 14 = Kóspál et al. (2016), 15 = Semkov et al. (2010), 16 = Magakian et al. (2013), 17 = Movsessian et al. (2003), 18 = Peneva et al. (2010), 19 = Reipurth et al. (2007), 20 = Semkov et al. (2019).
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