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Home All issues Volume 499 / No 2 (May IV 2009) A&A, 499 2 (2009) 515-527 Full HTML
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Table 6:

Circumstellar SiO fractional abundance, f0, and the radius of the SiO line-emitting region, $r_{\rm {e}}$, with 1$\sigma $-errors, from the best-fit model. The reduced $\chi ^{2}$ for the best-fit model and the number of observational constraints, N, are also given.

Source		 f0 $r_{\rm {e}}$ $\chi^{2}_{\rm red}$ N

R And		 $5.1\pm4.9\times10^{-5}$ $4.0\pm3.0\times10^{15}$ 0.6 5
W Aql $3.0\pm1.0\times10^{-6}$ $6.5\pm2.5\times10^{15}$ 0.2 4
S Cas $9.0\pm6.0\times10^{-6}$ $9.0\pm4.0\times10^{15}$ 7.2 3
WY Cas $1.2\pm0.3\times10^{-6}$ $1.3\pm0.7\times10^{16}$ 2.2 3
V386 Cep $7.5\pm2.5\times10^{-5}$ $3.0\pm2.0\times10^{15}$ 0.7 3
R Cyg $3.0\pm1.0\times10^{-6}$ $8.5\pm3.5\times10^{15}$ 1.2 4
$\chi $ Cyg $1.3\pm0.7\times10^{-5}$ $5.0\pm3.0\times10^{15}$ 5.2 4
R Gem $1.3\pm1.1\times10^{-5}$ $3.0\pm2.0\times10^{15}$ 1.1 3
RX Lac $1.8\pm0.8\times10^{-6}$ $3.6\pm2.4\times10^{15}$ 1.0 3
Y Lyn $1.9\pm1.1\times10^{-6}$ $3.5\pm1.5\times10^{15}$ 0.9 3
EP Vul $2.3\pm1.7\times10^{-5}$ $3.1\pm2.0\times10^{15}$ 0.7 3
AFGL 2425 $6.5\pm2.5\times10^{-6}$ $4.3\pm3.5\times10^{16}$ 1.2 3

Source LaTeX | All tables | In the text

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