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Table 1

Best-fit parameters from DUSTY models.

Source T* Tinn n τ550 log(Y) L Rinn Rout Mdust dust δ
(K) (K) (L) (1013cm) (1016cm) (10−6 M) (10−10 M yr−1)
EY Hya 3000200+100Mathematical equation: $3000^{+100}_{-200}$ 1350160+130Mathematical equation: $1350^{+130}_{-160}$ 1.860.06+0.05Mathematical equation: $1.86^{+0.05}_{-0.06}$ 0.350.09+0.16Mathematical equation: $0.35^{+0.16}_{-0.09}$ 3.80.4+0.7Mathematical equation: $3.8^{+0.7}_{-0.4}$ 5200±800 7.9 50 29 19 310
FH Vir 3400100+100Mathematical equation: $3400^{+100}_{-100}$ 1500150+150Mathematical equation: $1500^{+150}_{-150}$ 1.750.05+0.05Mathematical equation: $1.75^{+0.05}_{-0.05}$ 0.050.02+0.02Mathematical equation: $0.05^{+0.02}_{-0.02}$ 4.40.2+1.0Mathematical equation: $4.4^{+1.0}_{-0.2}$ 2100±300 3.3 83 13
IN Hya 3500200+100Mathematical equation: $3500^{+100}_{-200}$ 1450140+170Mathematical equation: $1450^{+170}_{-140}$ 1.780.05+0.07Mathematical equation: $1.78^{+0.07}_{-0.05}$ 0.040.02+0.03Mathematical equation: $0.04^{+0.03}_{-0.02}$ 4.00.2+1.0Mathematical equation: $4.0^{+1.0}_{-0.2}$ 1700±200 3.3 33 2.4
R LMi 3100200+100Mathematical equation: $3100^{+100}_{-200}$ 1250130+110Mathematical equation: $1250^{+110}_{-130}$ 2.030.04+0.04Mathematical equation: $2.03^{+0.04}_{-0.04}$ 1.60.2+0.3Mathematical equation: $1.6^{+0.3}_{-0.2}$ 4.60.2+0.8Mathematical equation: $4.6^{+0.8}_{-0.2}$ 3300±500 4.8 190 48 5.2 810
R UMa 3200400+100Mathematical equation: $3200^{+100}_{-400}$ 70080+120Mathematical equation: $700^{+120}_{-80}$ 2.130.04+0.06Mathematical equation: $2.13^{+0.06}_{-0.04}$ 0.400.10+0.12Mathematical equation: $0.40^{+0.12}_{-0.10}$ 4.00.4+0.8Mathematical equation: $4.0^{+0.8}_{-0.4}$ 5000±900 26 260 30 1.7 760
RR Eri 3300200+100Mathematical equation: $3300^{+100}_{-200}$ 800120+150Mathematical equation: $800^{+150}_{-120}$ 1.840.06+0.06Mathematical equation: $1.84^{+0.06}_{-0.06}$ 0.040.02+0.03Mathematical equation: $0.04^{+0.03}_{-0.02}$ 3.00.5+0.6Mathematical equation: $3.0^{+0.6}_{-0.5}$ 4700±900 20 20 3.2 6.0 680
RT Cnc 3300100+100Mathematical equation: $3300^{+100}_{-100}$ 1350140+140Mathematical equation: $1350^{+140}_{-140}$ 1.920.05+0.06Mathematical equation: $1.92^{+0.06}_{-0.05}$ 0.270.06+0.09Mathematical equation: $0.27^{+0.09}_{-0.06}$ 4.00.4+0.7Mathematical equation: $4.0^{+0.7}_{-0.4}$ 2100±300 4.2 42 5.5 3.0 230
RU Her* <2700 700130+140Mathematical equation: $700^{+140}_{-130}$ 1.980.06+0.05Mathematical equation: $1.98^{+0.05}_{-0.06}$ 0.200.07+0.14Mathematical equation: $0.20^{+0.14}_{-0.07}$ 3.40.4+0.7Mathematical equation: $3.4^{+0.7}_{-0.4}$ 20 000±5000 50 130 72 13 1230
RW Boo 3200300+100Mathematical equation: $3200^{+100}_{-300}$ 600100+170Mathematical equation: $600^{+170}_{-100}$ 1.900.09+0.14Mathematical equation: $1.90^{+0.14}_{-0.09}$ 0.060.03+0.06Mathematical equation: $0.06^{+0.06}_{-0.03}$ 4.00.1+1.0Mathematical equation: $4.0^{+1.0}_{-0.1}$ 2200±300 6.6 66 3.5 2.1 1670
RZ UMa 3100200+100Mathematical equation: $3100^{+100}_{-200}$ 1250120+150Mathematical equation: $1250^{+150}_{-120}$ 1.720.05+0.05Mathematical equation: $1.72^{+0.05}_{-0.05}$ 0.200.05+0.06Mathematical equation: $0.20^{+0.06}_{-0.05}$ 3.40.4+0.5Mathematical equation: $3.4^{+0.5}_{-0.4}$ 5100±1000 7.4 19 21 17 70
ST UMa 3400200+100Mathematical equation: $3400^{+100}_{-200}$ 1150110+170Mathematical equation: $1150^{+170}_{-110}$ 1.860.04+0.07Mathematical equation: $1.86^{+0.07}_{-0.04}$ 0.090.03+0.03Mathematical equation: $0.09^{+0.03}_{-0.03}$ 3.60.1+0.5Mathematical equation: $3.6^{+0.5}_{-0.1}$ 2900±500 7.5 30 4.0
SV Peg 2900200+200Mathematical equation: $2900^{+200}_{-200}$ 950100+160Mathematical equation: $950^{+160}_{-100}$ 1.720.06+0.10Mathematical equation: $1.72^{+0.10}_{-0.06}$ 0.200.07+0.13Mathematical equation: $0.20^{+0.13}_{-0.07}$ 3.00.5+0.3Mathematical equation: $3.0^{+0.3}_{-0.5}$ 10 000±2000 21 21 41 45 330
T Dra 2700200+100Mathematical equation: $2700^{+100}_{-200}$ 1200110+110Mathematical equation: $1200^{+110}_{-110}$ 2.000.03+0.03Mathematical equation: $2.00^{+0.03}_{-0.03}$ 4.50.5+1.0Mathematical equation: $4.5^{+1.0}_{-0.5}$ 4.80.4+0.7Mathematical equation: $4.8^{+0.7}_{-0.4}$ 13 000±3000 19 1200 1200 37 780
TU And 3200400+100Mathematical equation: $3200^{+100}_{-400}$ 1500120+180Mathematical equation: $1500^{+180}_{-120}$ 1.840.05+0.07Mathematical equation: $1.84^{+0.07}_{-0.05}$ 0.350.09+0.15Mathematical equation: $0.35^{+0.15}_{-0.09}$ 4.40.1+1.0Mathematical equation: $4.4^{+1.0}_{-0.1}$ 7500±1700 5.9 150 127
UY Leo 3300200+100Mathematical equation: $3300^{+100}_{-200}$ 1350140+160Mathematical equation: $1350^{+160}_{-140}$ 1.800.06+0.06Mathematical equation: $1.80^{+0.06}_{-0.06}$ 0.200.04+0.05Mathematical equation: $0.20^{+0.05}_{-0.04}$ 4.20.1+1.0Mathematical equation: $4.2^{+1.0}_{-0.1}$ 2000±300 4.0 64 23
V Eri 3000300+100Mathematical equation: $3000^{+100}_{-300}$ 1200140+140Mathematical equation: $1200^{+140}_{-140}$ 1.740.06+0.06Mathematical equation: $1.74^{+0.06}_{-0.06}$ 0.450.10+0.19Mathematical equation: $0.45^{+0.19}_{-0.10}$ 3.20.4+0.4Mathematical equation: $3.2^{+0.4}_{-0.4}$ 5100±1000 8.1 13 26 65 90
VY UMa 3100300+100Mathematical equation: $3100^{+100}_{-300}$ 1450130+160Mathematical equation: $1450^{+160}_{-130}$ 2.220.10+0.12Mathematical equation: $2.22^{+0.12}_{-0.10}$ 0.400.10+0.15Mathematical equation: $0.40^{+0.15}_{-0.10}$ 4.00.1+1.0Mathematical equation: $4.0^{+1.0}_{-0.1}$ 4700±900 6.1 24 0.15 0.050 40 000
VY UMa** 5.5
W Peg 3100400+100Mathematical equation: $3100^{+100}_{-400}$ 950120+150Mathematical equation: $950^{+150}_{-120}$ 2.030.05+0.05Mathematical equation: $2.03^{+0.05}_{-0.05}$ 0.350.11+0.16Mathematical equation: $0.35^{+0.16}_{-0.11}$ 4.00.3+0.8Mathematical equation: $4.0^{+0.8}_{-0.3}$ 5300±1000 15 150 26 4.1 1100
Y CrB 3100300+100Mathematical equation: $3100^{+100}_{-300}$ 1300120+160Mathematical equation: $1300^{+160}_{-120}$ 1.760.05+0.06Mathematical equation: $1.76^{+0.06}_{-0.05}$ 0.250.08+0.13Mathematical equation: $0.25^{+0.13}_{-0.08}$ 3.20.4+0.5Mathematical equation: $3.2^{+0.5}_{-0.4}$ 4500±800 6.4 64 7.5 8.1 160
Y Gem 3100200+100Mathematical equation: $3100^{+100}_{-200}$ 1250150+160Mathematical equation: $1250^{+160}_{-150}$ 1.700.07+0.06Mathematical equation: $1.70^{+0.06}_{-0.07}$ 0.030.02+0.03Mathematical equation: $0.03^{+0.03}_{-0.02}$ 2.80.7+0.5Mathematical equation: $2.8^{+0.5}_{-0.7}$ 8500±1800 9.2 5.8 1.0
Z Cnc 3200200+100Mathematical equation: $3200^{+100}_{-200}$ 1000180+200Mathematical equation: $1000^{+200}_{-180}$ 1.60.2+0.2Mathematical equation: $1.6^{+0.2}_{-0.2}$ 0.100.03+0.05Mathematical equation: $0.10^{+0.05}_{-0.03}$ 2.00.4+0.3Mathematical equation: $2.0^{+0.3}_{-0.4}$ 4200±600 12 1.2 1.1 11 55

Notes. Column 1: name of the source; Col. 2: stellar effective temperature; Col. 3: dust shell inner radius temperature; Col. 4: dust shell density power-law index; Col. 5: dust shell radial optical depth at 550 nm (from Rinn to Rout); Col. 6: logarithm of the dust shell outer-to-inner radii ratio; Col. 7: bolometric luminosity; Col. 8: dust shell inner radius; Col. 9: dust shell outer radius; Col. 10: dust shell mass; Col. 11: dust mas-loss rate; and Col. 12: gas-to-dust ratio. *In the case of RU Her, the sensitivity study indicates T* <2700K, although we noted that 2600 K fits the SED correctly (see Fig. 1). **In the case of VY UMa, the dust mass estimated for the detached shell is included separately.

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