EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 646 (February 2021) A&A, 646 (2021) A161 Full HTML
Free Access

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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.