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Table 1

Estimated masses and temperatures in the wind-ISM interaction regions based on the measured fluxes in the PACS 70 and 160 µm images and assuming agr = 0.1 µm.

Source Mask [″] [Jy] [Jy] Rfir ΔRfir [10–5 M] [K]
Carbon dust
AQ And 10 3.2 1.8 1.8 0.5 23.3 38
U Ant 20 22.0 6.2 3.6 1.1 3.9 52
UU Aur 40 6.0 3.3 1.8 0.6 6.5 39
U Cam (*) 30 4.3 4.5 1.0 0.3 23.7 32
RT Cap 40 1.0 1.4 0.8 0.2 4.0 30
S Cep (*) 20 2.5 1.0 2.5 0.8 2.1 44
Y CVn (*) 30 2.2 11.8 0.2 0.1 126.2 22
TTCyg 10 2.6 1.3 1.9 0.6 6.6 40
U Hya 30 28.9 14.7 2.0 0.6 10.2 40
CW Leo (*) 0 3459.6 598.6 5.8 1.8 42.8 70
WOri 45 1.2 0.3 2.0 0.6 0.3 55
WPic 20 1.2 0.3 1.4 0.4 0.6 55
TX Psc (*) 10 5.8 1.9 3.1 1.0 1.5 48
RScl 10 28.1 5.8 4.8 1.5 4.6 62
S Sct 20 17.3 14.9 1.2 0.4 62.8 33
X TrA (*) 20 7.6 7.4 1.0 0.3 13.3 32
 
Silicate dust
θ Aps 35 6.6 1.4 4.8 1.5 0.4 46
W Aql 30 9.6 3.3 2.9 0.9 7.6 43
EP Aqr 20 8.2 2.9 2.9 0.9 1.9 38
RCas 45 19.9 6.3 3.2 1.0 3.6 39
S Cas (*) 20 2.6 2.2 1.2 0.4 35.4 29
µ Cep 45 46.8 6.2 7.5 2.3 13.0 59
o Cet (*) 30 72.4 18.4 3.9 1.2 4.2 43
χ Cyg (*) 20 7.6 2.8 2.7 0.8 2.5 37
X Her (*) 20 10.4 3.4 3.1 1.0 2.2 39
RHya 55 11.3 5.5 2.1 0.6 3.8 34
W Hya 50 32.1 8.6 3.7 1.2 2.7 42
R Leo 50 20.7 3.3 6.4 2.0 0.3 53
T Mic (*) 20 7.4 2.4 3.1 0.9 3.7 39
α Ori (*) 200 77.9 31.3 2.5 0.8 23.3 36
XPav 30 9.3 4.5 2.1 0.6 16.5 34
V1943 Sgr 30 6.4 3.3 2.0 0.6 7.3 33
NML Tau 55 10.3 4.8 2.1 0.7 15.0 34
RT Vir 50 4.9 3.5 1.4 0.4 4.9 30

Notes. The observed FIR-ratio RFIR is given by . All corresponding PACS images and radiative transfer models are shown in Figs. A.1B.12. (*)Sources not modelled with radiative transfer (Sect. 3.2).

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