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Table A.1.

Best fitting parameters with corresponding reduced chi-squared, log-likelyhood, and BIC for the fitting of the three jet models to IRAS 19135+3937.

Jet model p(a) i θout θin c v0 vin vout cv Rprim χ2 BIC ΔBIC
(°) (°) (°) (km s−1) (km s−1) (km s−1) aprim
A 8 78.8 ± 0.8 75.9 ± 1.1 1.94 ± 0.14 1210 ± 90 11 ± 5 0.66 ± 0.04 0.2434 −24 878 0
4 78.5 ± 1.1 76.3 ± 0.9 2.16 ± 0.08 1010 ± 40 16 ± 4 0.68 ± 0.02 0.2461 −24 844 34
2 79.9 ± 1.1 77.8 ± 1.5 2.11 ± 0.12 1150 ± 170 18 ± 4 0.56 ± 0.03 0.2545 −24 738 140
B 8/2 79.5 ± 0.9 76.3 ± 0.8 76.2 ± 0.8 2.83 ± 0.04 1360 ± 30 82 ± 6 0.22 ± 0.07 0.565 ± 0.011 0.2433 −24 861 17
8/−2 79.5 ± 0.8 76.4 ± 0.9 76.3 ± 1.5 2.82 ± 0.13 1360 ± 30 77 ± 9 0.30 ± 0.12 0.559 ± 0.014 0.2428 −24 867 11
4/2 79.6 ± 0.8 77.2 ± 0.7 77.0 ± 0.8 2.46 ± 0.04 1240 ± 40 70 ± 4 0.61 ± 0.06 0.525 ± 0.013 0.2463 −24 824 54
4/−2 79.6 ± 0.7 77.3 ± 0.9 76.9 ± 0.9 2.47 ± 0.04 1240 ± 30 69 ± 4 0.60 ± 0.12 0.52 ± 0.02 0.2455 −24 833 45
2/−2 76.5 ± 0.9 75.1 ± 0.9 74.4 ± 1.1 2.39 ± 0.06 980 ± 20 82 ± 16 0.47 ± 0.10 0.56 ± 0.02 0.2517 −24 755 123
0/4 79.5 ± 0.8 77.6 ± 1.3 77.2 ± 1.6 2.05 ± 0.08 1360 ± 100 67 ± 9 0.83 ± 0.08 0.47 ± 0.06 0.2600 −24 651 227
C 8/2 75.6 ± 1.0 72.4 ± 1.3 70 ± 2 2.96 ± 0.06 1300 ± 60 59 ± 18 5 ± 4 0.65 ± 0.02 0.2536 −24 731 147
8/−2 75.6 ± 1.6 72 ± 3 68 ± 5 2.98 ± 0.16 1280 ± 80 61 ± 17 5 ± 5 0.657 ± 0.014 0.2790 −24 412 466
4/2 75.4 ± 1.2 73 ± 2 55 ± 11 2.4 ± 0.2 1340 ± 50 430 ± 50 19 ± 4 0.66 ± 0.03 0.2501 −24 776 102
4/−2 75.4 ± 0.7 73.0 ± 0.9 71.7 ± 1.4 2.63 ± 0.08 1220 ± 50 60 ± 20 12 ± 10 0.662 ± 0.013 0.2477 −24 805 73
2/−2 76.2 ± 0.9 74.9 ± 1.2 62.5 ± 1.0 2.48 ± 0.08 1310 ± 60 300 ± 20 27 ± 7 0.56 ± 0.03 0.2544 −24 722 156
0/4 75.3 ± 0.9 73.0 ± 1.1 44 ± 4 1.8 ± 0.2 1260 ± 40 760 ± 80 20 ± 5 0.67 ± 0.02 0.2491 −24 788 90

Notes. ΔBIC denotes the difference in BIC with the best-fitting model. The jet models are model A (the stellar jet model), model B (the disk-wind model), and model C (the X-wind model).

(a)

p for model A, pin and pout for model B and C.

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