Table B.1
Reference classification and υLSR for the FUors and EXors in our sample, including NH3 detections and non-detections.
| Name | Type | υLSR (km s−1) | υLSR (NH3) (km s−1) | Classification (Class 0 – II) | References | Distance* (pc) |
|---|---|---|---|---|---|---|
| RNO 1B/1C** | FUor | −17.83 (13CO) | −17.83 (0.02) | 1B: Class 0/II,1C: Class II | 1, 2 | 965 |
| V1180 Cas | EXor | – | – | – | – | 600 |
| V512 Per (SVS 13) | EXor | 8.35 (12CO) | 8.45 (0.01) | Class I | 3 | 275 |
| PP 13S | FUor | −3.5 (12CO) | −3.62 (0.01) | Class I | 4 | 350 |
| L1551 IRS 5 | FUor | 6.46 (13CO) | 6.35 (0.01) | Class I | 5, 6 | – |
| XZ Tau | EXor | 6.8 (12CO) | – | Class II | 7, 8 | 140 |
| UZ Tau E | EXor | – | – | Class II | 9 | 140 |
| VY Tau | EXor | + 18 or +19 (12CO) | – | Class II | 10 | 140 |
| LDN 1415 IRS | EXor | −5.2 (12CO) | −5.77 (0.02) | Class I | 11 | 170 |
| DR Tau | EXor | – | – | Class II | 12 | – |
| V582 Aur | FUor | −10.85 (13CO) | – | Class II | 5, 13 | – |
| V1118 Ori | EXor | – | – | Class II | 14 | 414 |
| Haro 5a IRS | FUor | 10.90 (13CO) | 10.7 (0.01) | Class 0/I | 5, 16 | 450 |
| NYOri | EXor | – | – | – | – | 414 |
| V1143 Ori | EXor | – | – | Class II | 17 | 500 |
| V883 Ori | FUor | 4.10 (13CO) | – | Class I | 5, 18 | 460 |
| HBC 494 | FUor | −4.6 (12CO) | – | Class I | 19 | – |
| V2775 Ori | FUor | 3.08 (13CO) | 3.05 (0.01) | late Class I | 5, 20 | 420 |
| FU Ori | FUor | 11.96 (13CO) | – | Class II | 5, 21 | 450 |
| V1647 Ori | FUor | 10.06 (13CO) | – | Class I/II | 5, 22, 23 | 400 |
| NGC 2071 | FUor | 9.2 (13CO) | 10.4 (0.01) | – | 24 | – |
| V899 Mon | FUor | 9.57 (13CO) | 9.63 (0.01) | Class II | 5, 25 | – |
| IRAS 06393+0913 | FUor | 4.3 (0.2) (12CO) | 7.72 (0.02) | Class I | 26, 27 | – |
| AR 6A/6B | FUor | 5.02 (13CO) | 5.06 (0.02) | Class II | 5, 28 | 800 |
| IRAS 06297+1021W | FUor | 5.1 (0.2) (12CO) | 4.17 (0.01) | Class I | 26, 27 | – |
| V900 Mon | FUor | 13.77 (13CO) | – | Class I | 5, 29, 30 | 1100 |
| V960 Mon | FUor | 23.81 (13CO) | 23.8 (0.02) | Class II | 5, 31 | – |
| ZCMa | FUor | 13.91 (13CO) | 13.8 (0.02) | Class I | 5, 32 | 1125 |
| iPTF 15AFQ | FUor | 14.04 (13CO) | 13.3 (0.01) | Class I | 5, 33 | – |
| IRAS 18270−0153W | FUor | – | 7.61 (0.01) | Class I | 34 | – |
| OO Ser | FUor | 8.36 (13CO) | 8.31 (0.01) | Class I | 5, 35 | 311 |
| IRAS 18341−0113S | FUor | – | 9.27 (0.01) | Class I | 34 | – |
| V371 Ser | EXor | – | 8.34 (0.01) | – | – | 311 |
| Parsamian 21 | FUor | 27 (Li I, Fe I) | – | Class I/II | 36 | 400 |
| Gala 18dvy | FUor | – | – | Class II | 37 | – |
| V1515 Cyg | FUor | 5.80 (13CO) | – | – | 1 | 1000 |
| PV Cep | EXor | −3 (nearby cloud) | – | – | 38 | 325 |
| V2492 Cyg | EXor | 4.97 (13CO) | 4.71 (0.02) | Class I | 1, 39 | 600 |
| HBC 722 | FUor | 4.05 (13CO) | 4.93 (0.01) | Class II | 1, 40 | 600 |
| V1057 Cyg | FUor | 4.3 (13CO) | 4.35 (0.02) | Class II | 1, 41 | 600 |
| V2495 Cyg | FUor | – | −3.83 (0.02) | Class I/II | 42 | 800 |
| RNO 127 | FUor | – | −2.90 (0.01) | – | – | 800 |
| CB 230 | FUor | 2.78 (N2H+) | 2.79 (0.01) | Class 0/I | 27, 43 | – |
| V1735 Cyg | FUor | 4.05 (13CO) | 3.80 (0.01) | Class II | 1, 44, 45 | 900 |
| HH 354 IRS | FUor | −1.1 (CS) | −1.52(0.01) | Class 0/I | 46, 47 | 750 |
| V733 Cep | FUor | −17.83 (13CO) | −8.93 (0.01) | Class II*** | 1, 27 | 800 |
Notes. The first column lists the name, the second the type of object, and the third and fourth columns list υLSR from literature observations (primarily of CO) and our υLSR derived from ammonia observations. The fifth column lists the classification (if available), sixth the references, and finally the distances. Errors are given in parentheses.
* – Adopted from Audard et al. (2014); exceptions are RNO 1B/1C (Bailer-Jones et al. 2021), V512 Per (Bailer-Jones et al. 2021), Z CMa (Dong et al. 2022), and HH 354 IRS (Reipurth et al. 1997). In these cases we detected water masers and adopted updated distance values in our Paper II.
** – RNO 1B/1C is counted into the Class II statistics in Sect. 4.2.
1 – Fehér et al. (2017), 2 – Quanz et al. (2007a), 3 – Diaz-Rodriguez et al. (2022), 4 – Sandell & Aspin (1998), 5 – Cruz-Sáenz de Miera et al. (2023), 6 – Fuller et al. (1995), 7 – ALMA Partnership et al. (2015), 8 – Zapata et al. (2015), 9 – Mathieu et al. (1996), 10 – Herbig (1990), 11 – Stecklum et al. (2007), 12 – Banzatti et al. (2014), 13 – Ábrahám et al. (2018), 14 – Giannini et al. (2016), 15 – Kóspál et al. (2017), 16 – Kóspál et al. (2021), 17 – Parsamian & Mujica (2004), 18 – White et al. (2019), 19 – Ruíz-Rodríguez et al. (2017), 20 – Zurlo et al. (2017), 21 – Herbig (1977), 22 – Ábrahám et al. (2004), 23 – Principe et al. (2018), 24 – Stojimirović et al. (2008), 25 – Park et al. (2021), 26 – Wouterloot & Brand (1989), 27 – Connelley & Reipurth (2018), 28 – Moriarty-Schieven et al. (2008), 29 – Reipurth et al. (2012), 30 – Takami et al. (2019), 31 – Kóspál et al. (2015), 32 – Gramajo et al. (2014), 33 – Miller et al. (2015), 34 – Connelley & Greene (2010), 35 – Kóspál et al. (2006), 36 – Kóspál et al. (2008), 37 – Szegedi-Elek et al. (2020), 38 – Torrelles et al. (1986), 39 – Hillenbrand et al. (2013), 40 – Kóspál et al. (2016), 41 – Szabó et al. (2021), 42 – Liu et al. (2018), 43 – Chen et al. (2007), 44 – Harvey et al. (2008), 45 – Kóspál et al. (2011), 46 – Bronfman et al. (1996), 47 – Reipurth & Aspin (1997)
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