Table D.3.
Results from our CO RD analysis (Sect. 6), including double-fit (hot and warm) components for NML Tau, χ Cyg, π Gru, W Aql, and IRAS 17347-3139.
| Target name | d (pc) | vexp (km s−1) | rCO (cm) | Trot (K) |
 (cm−2) |
MH2 (M⊙) | Ṁ (M⊙ yr−1) | CorrectionMH2 |
|---|---|---|---|---|---|---|---|---|
| RR Aql | 530 | 9.0 | 1 × 1015 | 460 ± 60 | (8.8 ± 3.0) × 1017 | (2.3 ± 0.8) × 10−5 | 7 × 10−7 | 1.2 |
| o Cet | 110 | 8.1 | 6 × 1014 | 530 ± 20 | (2.6 ± 0.3) × 1018 | (2.5 ± 0.3) × 10−5 | 10−6 | 1.6 |
| W Hya | 98 | 7.5 | 4 × 1014 | 550 ± 40 | (3.8 ± 1.0) × 1018 | (1.6 ± 0.4) × 10−5 | 9 × 10−7 | 1.6 |
| IRAS 20038-2722 | 197 | 5.4 | 4 × 1014 | 500 ± 20 | (1.4 ± 0.2) × 1018 | (5.9 ± 0.9) × 10−6 | 3 × 10−7 | 1.4 |
| T Cep | 190 | 5.5 | 1 × 1015 | 370 ± 40 | (6.3 ± 2.5) × 1017 | (1.7 ± 0.7) × 10−5 | 3 × 10−7 | 1.2 |
| NML Tau | 260 | 18.0 | 1 × 1015 | 490 ± 20 | (5.9 ± 1.0) × 1018 | (1.6 ± 0.3) × 10−4 | 9 × 10−6 | 1.5 |
| NML Tau | 260 | 18.0 | 1 × 1015 | 370 ± 20 | (9.5 ± 1.4) × 1018 | (2.5 ± 0.4) × 10−4 | 1 × 10−5 | – |
| NML Tau | 260 | 18.0 | 1 × 1015 | 820 ± 210 | (1.0 ± 0.9) × 1018 | (2.7 ± 2.4) × 10−5 | 2 × 10−6 | – |
| R Dor | 59 | 5.5 | 4 × 1014 | 520 ± 20 | (1.8 ± 0.2) × 1018 | (7.7 ± 0.8) × 10−6 | 3 × 10−7 | 1.5 |
| TX Cam | 380 | 18.5 | 2 × 1015 | 240 ± 10 | (4.4 ± 0.7) × 1018 | (4.7 ± 0.7) × 10−4 | 10−5 | 1.5 |
| X Her | 137 | 6.5 | 4 × 1014 | 570 ± 50 | (8.0 ± 1.8) × 1017 | (3.4 ± 0.8) × 10−6 | 2 × 10−7 | 1.2 |
| IRAS 19474-0744 | 810 | 13.6 | 2 × 1015 | 460 ± 40 | (2.1 ± 0.5) × 1018 | (2.3 ± 0.5) × 10−4 | 5 × 10−6 | 1.3 |
| T Mic | 290 | 4.8 | 6 × 1014 | 550 ± 30 | (1.8 ± 0.3) × 1018 | (1.7 ± 0.3) × 10−5 | 4 × 10−7 | 1.6 |
| R Cas | 176 | 10.5 | 1 × 1015 | 400 ± 20 | (1.2 ± 0.1) × 1018 | (3.1 ± 0.4) × 10−5 | 10−6 | 1.2 |
| EP Aqr | 114 | 10.0 | 4 × 1014 | 470 ± 20 | (1.3 ± 0.2) × 1018 | (5.6 ± 0.6) × 10−6 | 4 × 10−7 | 1.2 |
| NML Cyg | 620 | 33.0 | 2 × 1015 | 470 ± 20 | (1.2 ± 0.2) × 1019 | (1.3 ± 0.2) × 10−3 | 7 × 10−5 | 1.6 |
| χ Cyg | 149 | 8.5 | 6 × 1014 | 620 ± 10 | (3.7 ± 0.3) × 1018 | (1.2 ± 0.1) × 10−5 | 5 × 10−7 | 1.6 |
| χ Cyg | 149 | 8.5 | 6 × 1014 | 480 ± 20 | (4.9 ± 0.4) × 1018 | (1.6 ± 0.2) × 10−5 | 7 × 10−7 | – |
| χ Cyg | 149 | 8.5 | 6 × 1014 | 690 ± 30 | (2.3 ± 0.2) × 1018 | (7.3 ± 1.5) × 10−6 | 3 × 10−7 | – |
| π Gru | 152 | 10.0 | 6 × 1014 | 670 ± 20 | (4.0 ± 0.6) × 1018 | (1.3 ± 0.2) × 10−5 | 7 × 10−7 | 1.4 |
| π Gru | 152 | 10.0 | 6 × 1014 | 460 ± 20 | (7.1 ± 1.1) × 1018 | (2.3 ± 0.2) × 10−5 | 10−6 | – |
| π Gru | 152 | 10.0 | 6 × 1014 | 870 ± 30 | (1.3 ± 0.2) × 1018 | (4.2 ± 0.7) × 10−6 | 2 × 10−7 | – |
| W Aql | 395 | 16.5 | 2 × 1015 | 550 ± 10 | (2.9 ± 0.2) × 1018 | (1.0 ± 0.1) × 10−4 | 3 × 10−6 | 1.2 |
| W Aql | 395 | 16.5 | 2 × 1015 | 440 ± 10 | (3.9 ± 0.3) × 1018 | (1.4 ± 0.1) × 10−4 | 3 × 10−6 | – |
| W Aql | 395 | 16.5 | 2 × 1015 | 570 ± 20 | (2.3 ± 0.6) × 1018 | (7.9 ± 2.0) × 10−5 | 2 × 10−6 | – |
| WX Psc | 700 | 19.3 | 2 × 1015 | 560 ± 70 | (3.2 ± 1.0) × 1018 | (3.3 ± 1.0) × 10−4 | 10−5 | 1.0 |
| V1300 Aql | 620 | 16.5 | 2 × 1015 | 510 ± 20 | (1.8 ± 0.2) × 1018 | (1.9 ± 0.2) × 10−4 | 5 × 10−6 | 1.0 |
| OH 231.8+4.2 | 1500 | 15.0 | 4 × 1015 | 240 ± 40 | (3.5 ± 2.5) × 1018 | (1.5 ± 1.0) × 10−3 | 2 × 10−5 | 1.0 |
| OH 26.5+0.6 | 1370 | 17.0 | 4 × 1015 | 410 ± 100 | (2.4 ± 1.8) × 1018 | (1.0 ± 0.8) × 10−3 | 10−5 | 1.0 |
| IRAS 22036+5306 | 4000 | 30.0 | 6 × 1016 | 280 ± 20 | (1.0 ± 0.2) × 1017 | (9.6 ± 2.1) × 10−3 | 2 × 10−5 | 1.1 |
| AFGL 6815 | 2900 | 15.0 | 6 × 1016 | 310 ± 20 | (1.9 ± 0.4) × 1017 | (1.8 ± 0.3) × 10−2 | 10−5 | 1.1 |
| IRAS 17347-3139 | 3680 | 25.0 | 6 × 1016 | 630 ± 20 | (5.3 ± 0.7) × 1017 | (5.0 ± 0.6) × 10−2 | 7 × 10−5 | 1.0 |
| IRAS 17347-3139 | 3680 | 25.0 | 6 × 1016 | 480 ± 10 | (8.2 ± 0.4) × 1017 | (7.8 ± 0.4) × 10−2 | 10−4 | – |
| IRAS 17347-3139 | 3680 | 25.0 | 6 × 1016 | 820 ± 40 | (1.7 ± 0.4) × 1017 | (1.6 ± 0.4) × 10−2 | 2 × 10−5 | – |
| NGC 6302 | 1170 | 10.0 | 6 × 1016 | 280 ± 10 | (1.2 ± 0.2) × 1017 | (1.2 ± 0.2) × 10−2 | 6 × 10−6 | 1.1 |
| NGC 6537 | 1500 | 18.0 | 6 × 1016 | 200 ± 10 | (1.5 ± 0.4) × 1017 | (1.4 ± 0.4) × 10−2 | 10−5 | 1.0 |
Notes. Column 1: target name; Col. 2: distance to the source (d); Col. 3: expansion velocity of the gas (vexp); Col. 4: characteristic radius of the CO-emitting region adopted (rCO); Col. 5: rotational temperature (Trot); Col. 6: column density of CO (
); Col. 7: total mass of H2 within the CO-emitting volume (MH2); Col. 8: mass-loss rate (Ṁ = MH2 × vexp/rCO); and Col. 9: ratio between MH2 after and before the opacity correction was applied.
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