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Table B.2:

Observational results of circumstellar SiO(J = 2-1, v=1) emission.
Source $T_{\rm mb}$ $\sigma $ $T_{\rm mb} \times D^{2}$ prev.
  [K] [K] [K pc2]$^{\rm a}$ det.$^{\rm b}$
R And 0.52 0.016 $4.7 \times 10^{4}$ Y
W And 0.72 0.027 $5.7 \times 10^{4}$ Y
VX Aql $\cdots$ 0.047 $8.8 \times 10^{4}$ $\cdots$
W Aql 0.17 0.022 $9.0 \times 10^{3}$ Y
AA Cam $\cdots$ 0.022 $4.2 \times 10^{4}$ $\cdots$
S Cas 1.9 0.025 $3.7 \times 10^{5}$ Y
V365 Cas $\cdots$ 0.026 $3.0 \times 10^{4}$ $\cdots$
WY Cas 0.15 0.014 $5.4 \times 10^{4}$ $\cdots$
V386 Cep 0.70 0.019 $1.5 \times 10^{5}$ $\cdots$
AA Cyg $\cdots$ 0.023 $1.6 \times 10^{4}$ N
AD Cyg $\cdots$ 0.053 $1.5 \times 10^{5}$ $\cdots$
R Cyg $\cdots$ 0.008 $4.5 \times 10^{3}$ Y
$\chi $ Cyg 8.1 0.082 $9.8 \times 10^{4}$ Y
TV Dra 0.08 0.012 $1.2 \times 10^{4}$ N
DY Gem $\cdots$ 0.030 $4.2 \times 10^{4}$ $\cdots$
R Gem 0.19 0.015 $9.3 \times 10^{4}$ N
ST Her $\cdots$ 0.022 $6.0 \times 10^{3}$ $\cdots$
RX Lac $\cdots$ 0.032 $9.3 \times 10^{3}$ $\cdots$
R Lyn $\cdots$ 0.027 $6.0 \times 10^{4}$ Y
Y Lyn $\cdots$ 0.012 $2.4 \times 10^{3}$ Y
S Lyr $\cdots$ 0.037 $1.6 \times 10^{5}$ $\cdots$
FU Mon $\cdots$ 0.038 $6.9 \times 10^{4}$ N
EP Vul $\cdots$ 0.050 $3.9 \times 10^{4}$ Y
DK Vul $\cdots$ 0.043 $7.2 \times 10^{4}$ $\cdots$
$^{\it a}$ For the non-detections we use 3 $\sigma \times D^{2}$; $^{\rm b}$ from Jorissen & Knapp (1998)
and references therein.

Source LaTeX | All tables | In the text

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