Table A.5
MM3 SED fit results.
Grid spacing | lin | log | log | log | log | log | lin | lin | log | log | lin | lin | log | 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 | Rsub | ° | L⊙ | |||||
aer04B9J | 5842 | 16.5 | 6.75 | 11.5 | 15 720 | 0.0981 | 440 | 1.06 | − 0.205 | 9.29 | 7.28 × 10−21 | 1.16 | 40.4 | 1.09 × 10−23 | 3.35 | 60.5 | 7161 |
aer04B9J | 6799 | 17.1 | 6.75 | 11.5 | 15 720 | 0.0981 | 440 | 1.06 | − 0.205 | 9.29 | 7.28 × 10−21 | 1.16 | 40.4 | 1.09 × 10−23 | 3.35 | 52 | 7161 |
rlHDFVxN | 7251 | 16.6 | 6.07 | 9.32 | 15 680 | 0.0321 | 1216 | 1.13 | − 1.32 | 11.8 | 9.75 × 10−23 | 1.64 | 32.8 | 8.59 × 10−22 | 3.05 | 59.6 | 4639 |
aer04B9J | 7291 | 17.3 | 7.11 | 11.5 | 15 720 | 0.0981 | 440 | 1.06 | − 0.205 | 9.29 | 7.28 × 10−21 | 1.16 | 40.4 | 1.09 × 10−23 | 3.35 | 39.5 | 7161 |
aer04B9J | 7694 | 17.5 | 6.75 | 11.5 | 15 720 | 0.0981 | 440 | 1.06 | − 0.205 | 9.29 | 7.28 × 10−21 | 1.16 | 40.4 | 1.09 × 10−23 | 3.35 | 42.3 | 7161 |
Ipv9dWMM | 9668 | 22.7 | 6.4 | 11.4 | 16 700 | 0.0795 | 244 | 1.15 | − 0.161 | 13.2 | 2.19 × 10−24 | 1.79 | 11.4 | 1.17 × 10−22 | 1 | 56.7 | 8932 |
rlHDFVxN | 10 702 | 16.8 | 6.07 | 9.32 | 15 680 | 0.0321 | 1216 | 1.13 | − 1.32 | 11.8 | 9.75 × 10−23 | 1.64 | 32.8 | 8.59 × 10−22 | 3.05 | 47.8 | 4639 |
WFmZWZb5 | 10 838 | 28.6 | 6.07 | 13.9 | 13 460 | 0.0754 | 207 | 1.05 | − 0.924 | 13.6 | 2 × 10−22 | 1.23 | 16.9 | 1.53 × 10−22 | 1 | 34.8 | 5571 |
jZiuuzpK | 11 033 | 26.3 | 7.11 | 10.9 | 25 230 | 0.0653 | 1559 | 1.15 | − 1.72 | 4.11 | 7.1 × 10−23 | 1.45 | 14.4 | 2.63 × 10−23 | 1 | 55 | 42 775 |
MR8w9seO | 11 686 | 28 | 6.07 | 5.01 | 23 850 | 0.0321 | 287 | 1.14 | − 1.42 | 12.4 | 3.7 × 10−22 | 1.01 | 16.7 | 4.14 × 10−21 | 1 | 51.8 | 7170 |
Mean model | |||||||||||||||||
Mean | 19.9 | 6.53 | 10.5 | 16 672 | 0.0679 | 513 | 1.09 | − 0.678 | 9.91 | 6.66 × 10−22 | 1.33 | 30.9 | 6.3 × 10−23 | 2.25 | 50.6 | 7541 | |
Sigma | 4.28 | 1.06 | 1.26 | 1.18 | 1.6 | 1.86 | 0.0389 | 0.554 | 1.34 | 13.8 | 0.233 | 10.7 | 7.88 | 1.73 | 7.95 | 1.71 |
Notes. The table contains the full parameter set as well as the derived luminosities (see Sect. 5.2) for the ten best models, together with their respective
χ2 -values. The weighted mean and standard deviation σ
is given in the bottom. The confidence interval for log-sampled values extends from
to
x × σ, where for lin-spaced values it is x ± σ as usual. All masses (and densities) are given in unit dust mass, where we use the Weingartner & Draine (2001) Milky Way grain size distribution A for RV = 5.5. We note that, some models appear more than ones, but for different inclinations. In our analysis we thread them as different models. The envelope inner radius is set to
, its centrifugal radius rC
is set to
. All models extends to an outer radius, where density and temperature have dropped to the ambient level.
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