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Home All issues Volume 646 (February 2021) A&A, 646 (2021) A161 Full HTML
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Table A.6

MM1 SED fit results.

Grid spacing lin log log log log log lin lin log log lin lin log lin log
Model χ2 av d R* T* mdisk βdisk pdisk pcav inc L*
mag kpc R⊙ K M⊙ au au g/cc ° g/cc ° L⊙
Pre-burst
eGYXcOh8_02 42.8 67.6 7.11 3.79 25 590 0.000217 3110 1.18 − 0.131 2.34 5.25 × 10−19 1.56 31.5 1.81 × 10−23 19.3 5437
90Yt0exl_03 46.6 65.5 6.4 5.51 19 670 0.0357 1191 1.13 − 0.345 1.25 2.07 × 10−18 1.39 36.4 1.1 × 10−21 24.1 4017
PUyhjE8Z_02 47.5 48.2 6.75 14.1 12 130 4.01 × 10−8 278 1.28 − 1.46 11.4 2.07 × 10−17 1.76 23.4 2.71 × 10−22 11.3 3797
nTRTrE7X_02 51.2 59 7.11 2.71 29 889 8.1 × 10−6 423 1.13 − 0.607 1.85 9.58 × 10−18 1.94 32.7 4.99 × 10−21 18.1 5180
nTRTrE7X_03 55 47.5 6.75 2.71 29 889 8.1 × 10−6 423 1.13 − 0.607 1.85 9.58 × 10−18 1.94 32.7 4.99 × 10−21 23.3 5180
TJyUR9bA_02 57.8 62.6 7.11 3.91 23 840 3.1 × 10−7 631 1.17 − 0.102 12.7 7.15 × 10−18 1.89 46 9.4 × 10−23 14.4 4366
4kW1TtMH_04 59.1 41.8 6.4 47.3 7335 0.000299 140 1.24 − 0.752 2.49 5.14 × 10−17 1.35 32.9 8.17 × 10−22 30.6 5715
lQ0YS3aF_02 63.2 70 6.4 6.7 17 980 0.00527 3798 1.06 − 0.775 17.3 3.24 × 10−19 1.06 12.5 8.66 × 10−22 13.5 4150
qWHuujku_05 64.4 70 6.75 38 8551 2.63 × 10−5 1015 1.23 − 1.62 1.52 2.33 × 10−18 1.28 47.8 9.27 × 10−21 46.8 6832
qWHuujku_06 65.2 36.2 6.75 38 8551 2.63 × 10−5 1015 1.23 − 1.62 1.52 2.33 × 10−18 1.28 47.8 9.27 × 10−21 50 6832
Burst
90Yt0exl_L5.0 226 65.5 6.4 12.3 19 670 0.0357 1191 1.13 − 0.345 1.25 2.07 × 10−18 1.39 36.4 1.1 × 10−21 24.1 20 078
90Yt0exl_L5.5 229 65.5 6.4 12.9 19 670 0.0357 1191 1.13 − 0.345 1.25 2.07 × 10−18 1.39 36.4 1.1 × 10−21 24.1 22 081
eGYXcOh8_L4.5 234 67.6 7.11 8.04 25 590 0.000217 3110 1.18 − 0.131 2.34 5.25 × 10−19 1.56 31.5 1.81 × 10−23 19.3 24 470
eGYXcOh8_L5.0 234 67.6 7.11 8.47 25 590 0.000217 3110 1.18 − 0.131 2.34 5.25 × 10−19 1.56 31.5 1.81 × 10−23 19.3 27 185
90Yt0exl_L4.5 236 65.5 6.4 11.7 19 670 0.0357 1191 1.13 − 0.345 1.25 2.07 × 10−18 1.39 36.4 1.1 × 10−21 24.1 18 077
TJyUR9bA_L5.0 236 62.6 7.11 8.74 23 840 3.1 × 10−7 631 1.17 − 0.102 12.7 7.15 × 10−18 1.89 46 9.4 × 10−23 14.4 21 828
TJyUR9bA_L4.5 243 62.6 7.11 8.3 23 840 3.1 × 10−7 631 1.17 − 0.102 12.7 7.15 × 10−18 1.89 46 9.4 × 10−23 14.4 19 644
eGYXcOh8_L5.5 244 67.6 7.11 8.88 25 590 0.000217 3110 1.18 − 0.131 2.34 5.25 × 10−19 1.56 31.5 1.81 × 10−23 19.3 29 907
90Yt0exl_L6.0 245 65.5 6.4 13.5 19 670 0.0357 1191 1.13 − 0.345 1.25 2.07 × 10−18 1.39 36.4 1.1 × 10−21 24.1 24 108
qWHuujku_L4.5 245 36.2 6.75 80.7 8551 2.63 × 10−5 1015 1.23 − 1.62 1.52 2.33 × 10−18 1.28 47.8 9.27 × 10−21 50 30 745
Post-burst
lQ0YS3aF_L2.5 92.7 70 6.4 10.6 17 980 0.00527 3798 1.06 − 0.775 17.3 3.24 × 10−19 1.06 12.5 8.66 × 10−22 13.5 10 376
nTRTrE7X_L2.5 103 59 7.11 4.29 29 889 8.1 × 10−6 423 1.13 − 0.607 1.85 9.58 × 10−18 1.94 32.7 4.99 × 10−21 18.1 12 950
lQ0YS3aF_L3.0 105 70 6.4 11.6 17 980 0.00527 3798 1.06 − 0.775 17.3 3.24 × 10−19 1.06 12.5 8.66 × 10−22 13.5 12 448
90Yt0exl_L3.0 107 65.5 6.4 9.54 19 670 0.0357 1191 1.13 − 0.345 1.25 2.07 × 10−18 1.39 36.4 1.1 × 10−21 24.1 12 051
TJyUR9bA_L3.0 110 62.6 7.11 6.77 23 840 3.1 × 10−7 631 1.17 − 0.102 12.7 7.15 × 10−18 1.89 46 9.4 × 10−23 14.4 13 097
90Yt0exl_L2.5 110 65.5 6.4 8.71 19 670 0.0357 1191 1.13 − 0.345 1.25 2.07 × 10−18 1.39 36.4 1.1 × 10−21 24.1 10 044
nTRTrE7X_L3.0 114 59 7.11 4.69 29 889 8.1 × 10−6 423 1.13 − 0.607 1.85 9.58 × 10−18 1.94 32.7 4.99 × 10−21 18.1 15 540
TJyUR9bA_L3.5 114 62.6 7.11 7.32 23 840 3.1 × 10−7 631 1.17 − 0.102 12.7 7.15 × 10−18 1.89 46 9.4 × 10−23 14.4 15 281
eGYXcOh8_L2.5 116 67.6 7.11 5.99 25 590 0.000217 3110 1.18 − 0.131 2.34 5.25 × 10−19 1.56 31.5 1.81 × 10−23 19.3 13 591
nTRTrE7X_L2.0 118 59 7.11 3.83 29 889 8.1 × 10−6 423 1.13 − 0.607 1.85 9.58 × 10−18 1.94 32.7 4.99 × 10−21 18.1 10 362
Mean model
Mean 60.5 6.77 8.38* 16 834* 8.42 × 10−5 952 1.16 − 0.592 3.37 2.98 × 10−18 1.57 33.7 6.37 × 10−22 21.8 4984 (*)
Sigma 9.7 1.05 2.86 1.66 72.2 2.51 0.06 0.480 2.72 4.14 0.31 10.2 7.42 10.1 1.22

Notes. The table features the same structure as Table A.5, but additionally the burst-fit is included. The burst names are composed of the original model-name and the adapted luminosity increase. Consequently the weighted mean and σ are obtained taking into account both, the pre- and burst-results (see text). Only the parameters, which refers to the source are taken from the pre-burst alone (they change due to the burst). Again, the confidence interval for log-sampled values extends from to x × σ. We note that the inner radius of the disk is not a free parameter (unlike for MM3). Instead, it is governed by the sublimation radius (at Tsub = 1600 K). An outward shift of the sublimation radius may lower the dust masses for the post-/burst. (*) Pre-burst-value.

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