Table 4

Abundances of the observed species for IRAS 18095+2704 are presented for a model atmospheres of Teff = 6700 K, log g = 0.3 (KT), ξ = 6.0 and Teff = 6500 K, log g = 0.5, ξ = 4.7 (this work). The solar abundances from Asplund et al. (2009) is used to convert Klochkova's abundance of element X to [X/Fe] for comparison purposes.

SpeciesK95K95 This worklog ε
log ε(X)[X/Fe]log ε(X)[X/Fe]ΔN
C i8.27+0.507.92+0.40−0.35118.43
N i7.66+0.47≤7.19≤+0.27≤−0.4727.83
O i8.74+0.658.55+0.77−0.1968.69
Na i6.02+0.476.12+0.79+0.1056.24
Mg i7.42+0.627.14+0.45−0.2847.60
Mg ii7.52+0.727.17+0.48−0.3517.60
Al i5.81+0.124.86−0.68−0.9526.45
Si i7.48+0.717.18+0.58−0.3067.51
Si ii6.70+0.1017.51
S i6.96+0.536.98+0.77+0.0277.12
Ca i5.84+0.265.48+0.05−0.36136.34
Ca ii5.40−0.0346.34
Sc ii2.25−0.302.08−0.16−0.1773.15
Ti i5.68+1.443.97−0.07−1.7114.95
Ti ii4.05−0.194.04+0.00−0.01124.95
V ii3.45+0.233.24+0.22−0.2123.93
Cr i6.02+1.134.71−0.02−1.31105.64
Cr ii4.98+0.094.54−0.19−0.4495.64
Mn i5.12+0.514.44−0.08−0.6835.43
Fe i6.71−0.016.59+0.00−0.12317.50
Fe ii6.73+0.016.59+0.00−0.14117.50
Co i5.74+1.604.26+0.18−1.4814.99
Ni i6.13+0.665.48+0.17−0.65116.22
Cu i4.06+0.63≤3.35≤ +0.07≤−0.7114.19
Zn i4.60+0.783.86+0.21−0.7434.56
Sr ii2.52+0.5622.87
Y ii1.42−0.040.72−0.58−0.7042.21
Zr ii1.31−0.3632.58
Ba ii1.13−0.221.05−0.22−0.0812.18
La ii0.83+0.39≤0.31≤ +0.12≤−0.5211.10
Nd ii1.56+0.84≤0.44≤ −0.07≤−1.1211.42
Eu ii0.96+1.23−0.05+0.34−1.0110.52
SpeciesK95K95 This worklog ε
log ε(X)[X/Fe]log ε(X)[X/Fe]ΔN
C i8.27+0.507.92+0.40−0.35118.43
N i7.66+0.47≤7.19≤+0.27≤−0.4727.83
O i8.74+0.658.55+0.77−0.1968.69
Na i6.02+0.476.12+0.79+0.1056.24
Mg i7.42+0.627.14+0.45−0.2847.60
Mg ii7.52+0.727.17+0.48−0.3517.60
Al i5.81+0.124.86−0.68−0.9526.45
Si i7.48+0.717.18+0.58−0.3067.51
Si ii6.70+0.1017.51
S i6.96+0.536.98+0.77+0.0277.12
Ca i5.84+0.265.48+0.05−0.36136.34
Ca ii5.40−0.0346.34
Sc ii2.25−0.302.08−0.16−0.1773.15
Ti i5.68+1.443.97−0.07−1.7114.95
Ti ii4.05−0.194.04+0.00−0.01124.95
V ii3.45+0.233.24+0.22−0.2123.93
Cr i6.02+1.134.71−0.02−1.31105.64
Cr ii4.98+0.094.54−0.19−0.4495.64
Mn i5.12+0.514.44−0.08−0.6835.43
Fe i6.71−0.016.59+0.00−0.12317.50
Fe ii6.73+0.016.59+0.00−0.14117.50
Co i5.74+1.604.26+0.18−1.4814.99
Ni i6.13+0.665.48+0.17−0.65116.22
Cu i4.06+0.63≤3.35≤ +0.07≤−0.7114.19
Zn i4.60+0.783.86+0.21−0.7434.56
Sr ii2.52+0.5622.87
Y ii1.42−0.040.72−0.58−0.7042.21
Zr ii1.31−0.3632.58
Ba ii1.13−0.221.05−0.22−0.0812.18
La ii0.83+0.39≤0.31≤ +0.12≤−0.5211.10
Nd ii1.56+0.84≤0.44≤ −0.07≤−1.1211.42
Eu ii0.96+1.23−0.05+0.34−1.0110.52

Notes. K95: Klochkova (1995).

formula

N is the number of the lines employed in our abundance determination.

The solar abundances (log ε) are from Asplund et al. (2009).

Table 4

Abundances of the observed species for IRAS 18095+2704 are presented for a model atmospheres of Teff = 6700 K, log g = 0.3 (KT), ξ = 6.0 and Teff = 6500 K, log g = 0.5, ξ = 4.7 (this work). The solar abundances from Asplund et al. (2009) is used to convert Klochkova's abundance of element X to [X/Fe] for comparison purposes.

SpeciesK95K95 This worklog ε
log ε(X)[X/Fe]log ε(X)[X/Fe]ΔN
C i8.27+0.507.92+0.40−0.35118.43
N i7.66+0.47≤7.19≤+0.27≤−0.4727.83
O i8.74+0.658.55+0.77−0.1968.69
Na i6.02+0.476.12+0.79+0.1056.24
Mg i7.42+0.627.14+0.45−0.2847.60
Mg ii7.52+0.727.17+0.48−0.3517.60
Al i5.81+0.124.86−0.68−0.9526.45
Si i7.48+0.717.18+0.58−0.3067.51
Si ii6.70+0.1017.51
S i6.96+0.536.98+0.77+0.0277.12
Ca i5.84+0.265.48+0.05−0.36136.34
Ca ii5.40−0.0346.34
Sc ii2.25−0.302.08−0.16−0.1773.15
Ti i5.68+1.443.97−0.07−1.7114.95
Ti ii4.05−0.194.04+0.00−0.01124.95
V ii3.45+0.233.24+0.22−0.2123.93
Cr i6.02+1.134.71−0.02−1.31105.64
Cr ii4.98+0.094.54−0.19−0.4495.64
Mn i5.12+0.514.44−0.08−0.6835.43
Fe i6.71−0.016.59+0.00−0.12317.50
Fe ii6.73+0.016.59+0.00−0.14117.50
Co i5.74+1.604.26+0.18−1.4814.99
Ni i6.13+0.665.48+0.17−0.65116.22
Cu i4.06+0.63≤3.35≤ +0.07≤−0.7114.19
Zn i4.60+0.783.86+0.21−0.7434.56
Sr ii2.52+0.5622.87
Y ii1.42−0.040.72−0.58−0.7042.21
Zr ii1.31−0.3632.58
Ba ii1.13−0.221.05−0.22−0.0812.18
La ii0.83+0.39≤0.31≤ +0.12≤−0.5211.10
Nd ii1.56+0.84≤0.44≤ −0.07≤−1.1211.42
Eu ii0.96+1.23−0.05+0.34−1.0110.52
SpeciesK95K95 This worklog ε
log ε(X)[X/Fe]log ε(X)[X/Fe]ΔN
C i8.27+0.507.92+0.40−0.35118.43
N i7.66+0.47≤7.19≤+0.27≤−0.4727.83
O i8.74+0.658.55+0.77−0.1968.69
Na i6.02+0.476.12+0.79+0.1056.24
Mg i7.42+0.627.14+0.45−0.2847.60
Mg ii7.52+0.727.17+0.48−0.3517.60
Al i5.81+0.124.86−0.68−0.9526.45
Si i7.48+0.717.18+0.58−0.3067.51
Si ii6.70+0.1017.51
S i6.96+0.536.98+0.77+0.0277.12
Ca i5.84+0.265.48+0.05−0.36136.34
Ca ii5.40−0.0346.34
Sc ii2.25−0.302.08−0.16−0.1773.15
Ti i5.68+1.443.97−0.07−1.7114.95
Ti ii4.05−0.194.04+0.00−0.01124.95
V ii3.45+0.233.24+0.22−0.2123.93
Cr i6.02+1.134.71−0.02−1.31105.64
Cr ii4.98+0.094.54−0.19−0.4495.64
Mn i5.12+0.514.44−0.08−0.6835.43
Fe i6.71−0.016.59+0.00−0.12317.50
Fe ii6.73+0.016.59+0.00−0.14117.50
Co i5.74+1.604.26+0.18−1.4814.99
Ni i6.13+0.665.48+0.17−0.65116.22
Cu i4.06+0.63≤3.35≤ +0.07≤−0.7114.19
Zn i4.60+0.783.86+0.21−0.7434.56
Sr ii2.52+0.5622.87
Y ii1.42−0.040.72−0.58−0.7042.21
Zr ii1.31−0.3632.58
Ba ii1.13−0.221.05−0.22−0.0812.18
La ii0.83+0.39≤0.31≤ +0.12≤−0.5211.10
Nd ii1.56+0.84≤0.44≤ −0.07≤−1.1211.42
Eu ii0.96+1.23−0.05+0.34−1.0110.52

Notes. K95: Klochkova (1995).

formula

N is the number of the lines employed in our abundance determination.

The solar abundances (log ε) are from Asplund et al. (2009).

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