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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 rpol,SiMathematical equation: $r^-_{\text{{{pol}}, Si}}$ rpol,aCMathematical equation: $r^-_{\text {{pol}}, aC}$ Ω [Si][H]Mathematical equation: $\frac{[\rm{Si}]}{[\rm{H}]}$ [C][H]Mathematical equation: $\frac{[\rm{C}]}{[\rm{H}]}$ (τsμτt)VMathematical equation: $\left(\frac{\tau_{\rm {s}\upmu}}{\tau_{\rm {t}}}\right)_{\rm V}$
(%) (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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