Table 2
Dust parameters of the 27 sightlines that have been modelled.
| 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Star | a/b | Vvac | mμA | mSi | mvSi | maC | mvgr | mPAH | q | ![]() |
![]() |
Ω | ![]() |
![]() |
![]() |
| (%) | (nm) | (°) | (ppm) | (%) | |||||||||||
| HD 027778 | 2.0 | 10 | 25 | 37 | 28 | 5 | 3 | 1 | 2.3 | 112 | – | 38 | 42 | 78 | 20 |
| HD 037903 | 2.0 | 10 | 33 | 31 | 18 | 13 | 4 | 1 | 2.1 | 143 | 69 | 50 | 32 | 108 | 37 |
| HD 038023 | 1.5 | 5 | 32 | 37 | 19 | 8 | 2 | 2 | 2.6 | 25 | – | 53 | 38 | 88 | 34 |
| HD 046223 | 1.5 | 5 | 30 | 33 | 24 | 8 | 4 | 1 | 2.6 | 136 | – | 63 | 37 | 91 | 29 |
| HD 054439 | 1.5 | 5 | — | 58 | 21 | 13 | 5 | 3 | 2.8 | 112 | 69 | 27 | 38 | 93 | 0 |
| HD 062542 | 1.5 | 5 | 25 | 28 | 35 | 8 | 3 | 1 | 2.8 | 143 | – | 76 | 49 | 110 | 22 |
| HD 070614 | 2.0 | 10 | – | 52 | 22 | 18 | 6 | 2 | 2.5 | 143 | 42 | 47 | 34 | 109 | 0 |
| HD 091824 | 2.0 | 10 | 41 | 33 | 14 | 9 | 2 | 1 | 2.3 | 102 | – | 51 | 36 | 96 | 52 |
| HD 092044 | 2.0 | 10 | 34 | 36 | 19 | 8 | 2 | 1 | 2.6 | 112 | 88 | 39 | 38 | 89 | 48 |
| HD 093222 | 1.5 | 5 | 35 | 34 | 13 | 15 | 2 | 1 | 2.5 | 30 | – | 41 | 32 | 110 | 38 |
| HD 108927 | 2.0 | 10 | 30 | 32 | 20 | 13 | 4 | 1 | 2.0 | 97 | – | 46 | 33 | 106 | 23 |
| HD 110946 | 2.0 | 10 | 19 | 39 | 27 | 10 | 4 | 1 | 2.8 | 143 | 54 | 49 | 37 | 92 | 9 |
| HD 112607 | 1.5 | 5 | – | 39 | 39 | 13 | 6 | 3 | 2.7 | 143 | – | 37 | 35 | 96 | 0 |
| HD 112954 | 2.0 | 10 | 8 | 32 | 44 | 10 | 5 | 1 | 2.5 | 183 | 54 | 60 | 43 | 94 | 1 |
| HD 129557 | 1.5 | 5 | 35 | 44 | 12 | 3 | 4 | 2 | 2.0 | 102 | – | 47 | 41 | 81 | 42 |
| HD 146285 | 1.5 | 5 | 39 | 31 | 10 | 15 | 4 | 1 | 2.0 | 143 | 69 | 61 | 28 | 114 | 33 |
| HD 152245 | 1.5 | 5 | 35 | 38 | 14 | 8 | 3 | 2 | 2.6 | 112 | 88 | 40 | 37 | 91 | 44 |
| HD 152249 | 1.5 | 5 | 63 | 21 | 9 | 5 | 1 | 1 | 2.3 | 201 | 92 | 40 | 38 | 94 | 44 |
| HD 170740 | 1.5 | 5 | – | 46 | 29 | 16 | 6 | 3 | 2.8 | 183 | 26 | 72 | 35 | 103 | 0 |
| HD 185418 | 1.5 | 5 | 27 | 43 | 13 | 10 | 5 | 2 | 2.5 | 112 | 88 | 32 | 35 | 98 | 19 |
| HD 287150 | 2.0 | 10 | 17 | 32 | 34 | 13 | 3 | 1 | 2.8 | 143 | 8 | 36 | 36 | 97 | 6 |
| HD 294304 | 1.5 | 5 | 27 | 36 | 23 | 10 | 3 | 1 | 2.7 | 102 | – | 34 | 37 | 95 | 23 |
| HD 303308 | 2.0 | 10 | 26 | 38 | 23 | 9 | 3 | 1 | 2.4 | 112 | 88 | 52 | 39 | 88 | 20 |
| HD 315021 | 1.5 | 5 | 33 | 40 | 10 | 13 | 3 | 1 | 2.4 | 118 | – | 30 | 35 | 103 | 35 |
| HD 315023 | 1.5 | 5 | 32 | 38 | 11 | 15 | 2 | 2 | 2.5 | 143 | 88 | 53 | 33 | 108 | 32 |
| HD 315024 | 1.5 | 5 | 67 | 15 | 7 | 8 | 2 | 1 | 2.3 | 47 | – | 53 | 45 | 170 | 46 |
| HD 315032 | 2.0 | 5 | 34 | 33 | 17 | 11 | 4 | 1 | 2.3 | 112 | – | 16 | 34 | 104 | 43 |
| median | 31 | 37 | 19 | 10 | 3 | 1 | 2.5 | 118 | 69 | 37 | 96 | 32 | |||
| sigma | 16 | 8 | 9 | 4 | 1 | 1 | 0.3 | 23 | 25 | 4 | 17 | 17 | |||
Notes. For HD 091824 and HD 146285, the maximum grain size is r+ = 3 μm; otherwise, r+ = 1 μm. The derived C and Si abundances in the grains and the contribution of micrometre-sized dust agglomerates to the total optical depth are specified in Cols. 14-16. The median values and 1σ variations of the parameters are provided, excluding r-polsi for the two stars HD 038023 and HD 093222, as they exhibit peculiar polarisation spectra peaking in the B band.
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![Mathematical equation: $\frac{[\rm{Si}]}{[\rm{H}]}$](/articles/aa/full_html/2026/05/aa55848-25/aa55848-25-eq62.png)
![Mathematical equation: $\frac{[\rm{C}]}{[\rm{H}]}$](/articles/aa/full_html/2026/05/aa55848-25/aa55848-25-eq63.png)
