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Table 4

Best-fit values for our Cepheid sample.

Stars φ log g θ LD T eff M cse T cse χ 2
(mas) (K) (M) (K)

FF Aql 0.62 2.05 0.86 ± 0.03 5890 ± 235 1.8 ± 0.5 × 10-9 539 ± 53 0.41
AX Cir 0.27 2.00 0.76 ± 0.03 5911 ± 184 7.4 ± 5.9 × 10-10 712 ± 61 0.42
X Sgr 0.72 2.00 1.30 ± 0.04 5738 ± 314 3.0 ± 0.6 × 10-9 703 ± 52 0.74
η Aql 0.47 1.80 1.86 ± 0.12 5431 ± 498 1.0 ± 0.7 × 10-8 545 ± 60 1.01
W Sgr 0.48 1.70 1.14 ± 0.06 5632 ± 162 1.7 ± 0.4 × 10-9 853 ± 55 1.45
Y Oph 0.73 1.80 1.24 ± 0.05 5870 ± 387 3.9 ± 0.8 × 10-9 1419 ± 148 1.49
U Car 0.49 1.20 0.90 ± 0.02 4823 ± 52 4.4 ± 2.1 × 10-9 746 ± 94 0.70
SV Vul 0.04 1.40 0.76 ± 0.01 5744 ± 144 3.9 ± 7.4 × 10-8 620 ± 50 1.13

R Sct 0.48 0.00 1.74 ± 0.06 4605 ± 119 1486 ± 335 1.79
772 ± 82
AC Her 0.14 0.50 0.30 ± 0.02 5711 ± 293 286 ± 32 0.91
κ Pav 0.90 1.20 1.09 ± 0.05 6237 ± 119 9.9 ± 2.5 × 10-10 695 ± 36 0.30

Notes. φ is the pulsation phase. θLD and Teff are the photospheric fitted parameters, while Tcse is the CSE fitted parameter. Mcse is the total mass (dust + gas) of the CSE estimated using a gas to dust ratio of  ~100. For R Sct, the first line denotes the compact component. The χ2 has been estimated from the fit of the photospheric flux. See the text for the references of the effective gravity.

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