Table B.2
Fit results of the M-star sample.
| Identifier | Teff/ log g | Grain size and type | L | τ 0.5 | Ṁ | f | T c | f | p | f | R out | χ 2 |
| (K/–) | (L⊙) | (M⊙ yr-1) | (K) | (× 103) | ||||||||
|
|
||||||||||||
| wohg17 | 3300/+0.5 | a0.10 Oliv70 AlOx30 Fe30 | 932 967 | 1.201e-01 | 2.84e-07 | 1 | 1000 | 0 | 2.00 | 0 | 13 | 504 |
| msxlmc1212 | 3900/+0.5 | a0.20 Oliv40 AlOx60 Fe1 | 262 501 | 1.000e-04 | 1.14e-10 | 0 | 1000 | 0 | 2.00 | 0 | 13 | 98 |
| rsmen | 2500/+0.0 | a0.10 Oliv60 AlOx40 Fe30 | 752 101 | 2.044e-01 | 4.37e-07 | 1 | 1000 | 0 | 2.00 | 0 | 13 | 492 |
| w60d29 | 3800/+0.5 | a0.20 Oliv90 AlOx10 Fe30 | 350 174 | 1.000e-04 | 8.50e-11 | 0 | 1000 | 0 | 2.00 | 0 | 13 | 218 |
| hd269788 | 4250/+0.0 | a0.20 Oliv40 AlOx60 Fe3 | 611 699 | 3.000e-03 | 8.67e-09 | 0 | 760 | 1 | 2.00 | 0 | 13 | 4010 |
| msxlmc946 | 3200/+0.5 | a0.10 Oliv50 AlOx50 Fe30 | 339 561 | 4.252e-02 | 6.53e-08 | 1 | 1000 | 0 | 2.00 | 0 | 13 | 51 |
| hd269924 | 3600/+0.0 | a0.10 Oliv40 AlOx60 Fe3 | 745 922 | 1.000e-03 | 3.69e-09 | 0 | 1000 | 0 | 2.00 | 0 | 13 | 4892 |
| msxlmc1677 | 2700/+0.0 | a0.10 Oliv90 AlOx10 Fe30 | 1 952 457 | 6.687e-01 | 2.05e-06 | 1 | 1000 | 0 | 2.00 | 0 | 13 | 1315 |
| hd271832 | 3400/+0.0 | a0.50 Oliv80 AlOx20 Fe3 | 1 997 701 | 1.391e-03 | 4.90e-09 | 1 | 1000 | 0 | 2.00 | 0 | 13 | 2553 |
| msxlmc1686 | 2500/+0.0 | a0.20 Oliv70 AlOx30 Fe30 | 1 532 676 | 2.973e-01 | 4.86e-07 | 1 | 1000 | 0 | 2.00 | 0 | 13 | 270 |
| msxsmc067 | 3500/+0.0 | a0.10 Oliv50 AlOx50 Fe30 | 143 486 | 1.067e-02 | 1.12e-08 | 1 | 1000 | 0 | 2.00 | 0 | 13 | 196 |
| smc010889 | 3700/+0.5 | a0.10 Oliv70 AlOx30 Fe30 | 184 822 | 5.192e-02 | 6.01e-08 | 1 | 1000 | 0 | 2.00 | 0 | 10 | 697 |
| smc011709 | 3800/+0.5 | a0.20 Oliv40 AlOx60 Fe30 | 114 473 | 1.000e-02 | 9.16e-09 | 0 | 825 | 1 | 2.00 | 0 | 10 | 47 |
| pmmr24 | 3800/+0.5 | a0.50 Oliv60 AlOx40 Fe30 | 90 740 | 9.816e-02 | 6.28e-08 | 1 | 1000 | 0 | 2.00 | 0 | 10 | 52 |
| msxsmc096 | 3700/+0.5 | a0.50 Oliv60 AlOx40 Fe30 | 107 095 | 4.938e-02 | 3.35e-08 | 1 | 1000 | 0 | 2.00 | 0 | 13 | 76 |
| msxsmc109 | 3800/+0.5 | a0.10 Oliv90 AlOx10 Fe30 | 122 980 | 1.344e-01 | 1.21e-07 | 1 | 1000 | 0 | 2.00 | 0 | 13 | 245 |
| msxsmc168 | 3800/+0.5 | a0.10 Oliv90 AlOx10 Fe30 | 93 615 | 5.390e-02 | 4.21e-08 | 1 | 1000 | 0 | 2.00 | 0 | 13 | 320 |
| s3mc203963 | 3900/+0.5 | a0.20 Oliv40 AlOx60 Fe1 | 24 445 | 1.289e-03 | 4.49e-10 | 0 | 1000 | 0 | 2.00 | 0 | 13 | 160 |
| s3mc204111 | 4000/+0.0 | a0.20 Oliv50 AlOx50 Fe30 | 57 989 | 3.000e-03 | 1.25e-09 | 0 | 1000 | 0 | 2.00 | 0 | 13 | 7 |
| s3mc205104 | 4000/+0.0 | a0.20 Oliv40 AlOx60 Fe1 | 27 422 | 1.000e-04 | 3.74e-11 | 0 | 1000 | 0 | 2.00 | 0 | 13 | 17 |
Notes. Column 1 lists the identifier. Column 2 lists the information on the model atmosphere that is used as Teff (in K)/log g. Column 3 indicates the grain size and type: The number after the a indicates the grain size in μm. Then follows the proportion of olivine (MgFeSiO4), corundum, metallic iron, and sometimes forsterite. Column 4 lists the luminosity. Column 5 lists the dust optical depth at 0.5 μm, and Col. 6 lists the total mass-loss rate (assuming an expansion velocity of 10 km s-1, and a dust-to-gas ratio of 0.005). Column 7 indicates if the optical depth was fitted (f = 1, or fixed f = 0). Column 8 lists the temperature at the inner dust radius, and Col. 9 indicates if this temperature was fitted (f = 1, or fixed f = 0). Column 10 lists the slope of the density law, and Col. 11 indicates if this temperature was fitted (f = 1, or fixed f = 0). Column 12 lists the outer radius in units of the inner dust radius. Column 13 lists the reduced χ2 of the fit. The full table is available at the CDS.
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.