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Table 3.

DUSTY results for the VLBI sources.

Source rVLBI T⋆ Tdust τ10 PL*
[pc] [pc] [pc] [L⊙] [L⊙] [L⊙] [K] [K]
Miras
AP Lyn 501 10 10 4200 100 200 2900 700 0.28 No
BX Cam 579 10 10 7700 200 200 3000 1000 0.8 Yes
FV Boo 1034 60 67 1900 200 200 3000 700 0.3 No
NSV 17351 4064 157 168 25 600 1400 1600 3100 1000 1.2 No
OZ Gem 1246 58 63 2500 100 200 2700 600 0.7 No
QX Pup 1652 78 86 1300 100 100 3600 600 5.0 No
R Aqr 220 11 12 8100 600 600 2900 1200 0.14 Yes
R Cnc 266 19 22 4800 500 600 2900 600 0.02 Yes
R Hya 126 2 3 10 300 300 300 3100 1200 0.04 Yes
R Peg 374 36 44 4600 600 700 2900 1200 0.11 Yes
R UMa 508 12 14 4100 100 200 3000 1200 0.17 Yes
RR Aql 411 11 12 3500 100 200 2900 900 0.26 Yes
S CrB 424 28 33 8600 900 800 2900 1000 0.07 Yes
S Ser 801 25 27 5800 300 300 3000 600 0.04 Yes
SY Aql 922 56 64 2800 200 300 3000 700 0.24 No
SY Scl 1330 50 55 5700 300 300 3000 800 0.18 Yes
U Her 271 19 21 5800 600 600 2900 1000 0.08 Yes
T Lep 327 4 4 6100 200 100 2900 1200 0.06 Yes
U Lyn 792 36 39 6000 400 400 3000 900 0.16 Yes
UX Cyg 1918 198 250 4000 600 700 3600 600 5.0 No
V837 Per 918 9 8 5400 100 100 3100 1200 1.0 Yes
W Leo 971 18 19 6800 200 200 2600 600 0.04 Yes
X Hya 484 11 12 3800 100 100 3000 900 0.09 Yes
Y Lib 1173 64 73 3200 200 300 3000 700 0.06 Yes
SRa
HU Pup 3437 426 51 29 950 3450 3450 2600 600 0.48 No
RW Lep 636 59 72 10 300 1400 1500 3000 600 0.02 No
SRb and U
BX Eri 476 23 25 6500 400 500 3100 600 0.03 No
HS UMa 356 11 13 6100 300 300 3100 600 0.03 No
RT Vir 227 6 7 7400 300 300 3100 600 0.02 No
RX Boo 139 9 11 4700 500 600 3100 600 0.02 No
S Crt 433 23 25 4800 400 400 3200 600 0.01 No
SV Peg 334 7 7 8700 300 400 3100 600 0.02 No
V637 Per 1065 22 23 4500 200 200 3100 600 0.04 No

Notes. SRa/b: semi-regular a or b, U: unknown. rVLBI the median distance obtained with the VLBI parallax. the lower/upper uncertainties on the VLBI distance. the median luminosity; the lower/upper uncertainties on the luminosity. T⋆ is the stellar temperature; Tdust the dust temperature; τ10 the optical depth at 10 μm; *included in the PL derivation.

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