All Figures

$\begin{figure} \par\mbox{\includegraphics[width=8.8cm,clip]{3850f1a.eps}\hspace*{3mm} \includegraphics[width=8.8cm,clip]{3850f1b.eps} }\end{figure}$ Figure 1: [X/Fe] vs. $T_{\rm eff}$ and [X/Fe] vs. $\log~g$ . Triangles and asterisks are planet host and comparison sample stars, respectively. Dotted lines represent the solar value. The slopes represent linear least-squares fits to both planet-hosts and comparison stars.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{3850f2.eps} \end{figure}$ Figure 2: Distributions of planet-host stars and non-planet-host stars as functions of $T_{\rm eff}$ . The planet-host stars and the comparison sample are represented with solid and dotted lines, respectively.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3850f3.eps} \end{figure}$ Figure 3: [X/H] distributions for Ti, V and Co for the two subsamples of planet host (solid line) and comparison sample (dotted lines) stars with the same $T_{\rm eff}$ distributions.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=14.2cm,clip]{3850f4.eps} \end{figure}$ Figure 4: Comparison of the abundances of nine refractory elements calculated with EW values measured from spectra taken with different instruments. Along the x-asis are results from FEROS spectra, while along the y-axis we represent abundance values for the same objects, calculated using other spectra. UVES, CORALIE and SARG results are respectively represented with rhombi (HD 16141, HD 27442), triangles (HD 83443, HD 92788, HD 106252, HD 114386) and asterisks (HD 114783, HD 147513).
Open with DEXTER

In the text

$\begin{figure} \par\mbox{\includegraphics[width=5.8cm,clip]{3850f5a.eps}\hspace*... ...ps}\hspace*{2mm} \includegraphics[width=5.8cm,clip]{3850f5c.eps} }\end{figure}$ Figure 5: [X/H] vs. [Fe/H] for Si, Ca, Ti ( left), for Sc, Mn and V ( centre), for Cr, Co and Ni ( right). Triangles and asterisks represent stars with planetary-mass companion and "single'' field stars, respectively. The intersection of the dotted lines indicates solar value.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=15.6cm,clip]{3850f6.eps} \end{figure}$ Figure 6: [X/H] distribution for each element. The planet-host stars and the comparison sample are represented with solid and dotted lines, respectively.
Open with DEXTER

In the text

$\begin{figure} \par\mbox{\includegraphics[width=8.8cm,clip]{3850f7a.eps}\hspace*... ...ps}\hspace*{2mm} \includegraphics[width=8.8cm,clip]{3850f7d.eps} }\end{figure}$ Figure 7: [X/Fe] vs. [Fe/H](in dex) for $\alpha$ elements (Si, Ca, Ti, Sc) and for iron-peak elements (Cr, Co, Ni, Mn, V). [V/Fe] vs. [Fe/H] for $T_{\rm eff} > 5000$ K objects only ( below right panel). The triangles and asterisks represent stars with planets and "single'' stars, respectively. The intersection of the dotted lines indicates the solar value.
Open with DEXTER

In the text

$\begin{figure} \par\mbox{\includegraphics[width=5.6cm,clip]{3850f8a.eps}\hspace*... ...ps}\hspace*{2mm} \includegraphics[width=5.6cm,clip]{3850f8c.eps} }\end{figure}$ Figure 8: [X/Fe] vs. [Fe/H] trends using binned average values. The bins are 0.2 dex wide, centred on [Fe/H ] =-0.6, -0.4,-0.2,0,0.2 and 0.4 for both samples. Triangles are planet-hosts while rhombi are stars without a planetary-mass companion. The error bars represent the standard deviation about the mean value.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=16cm,clip]{3850f9.eps} \end{figure}$ Figure 9: Same as Fig. 6 but for the Na, Mg and Al distributions.
Open with DEXTER

In the text

$\begin{figure} \par\mbox{\includegraphics[width=8cm,clip]{3850f10a.eps}\hspace*{4mm} \includegraphics[width=8cm,clip]{3850f10b.eps} }\end{figure}$ Figure 10: [X/Fe] vs. [Fe/H] (in dex). Results by Beirão et al. (2005) with the addition of abundances from new comparison sample spectra. On the left are the plots for Na, Mg and Al, and on the right the same plots only for $T_{\rm eff} > 5000$ K objects. Triangles and asterisks represent stars with planetary-mass companions and "single'' field stars, respectively. The intersection of the dotted lines indicates the solar value.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{3850f11.eps} \end{figure}$ Figure 11: The same as Fig. 8 but for Na, Mg and Al.
Open with DEXTER

In the text

$\begin{figure} \par\mbox{\includegraphics[width=8.8cm,clip]{3850f1a.eps}\hspace*{3mm} \includegraphics[width=8.8cm,clip]{3850f1b.eps} }\end{figure}$	Figure 1: [X/Fe] vs. $T_{\rm eff}$ and [X/Fe] vs. $\log~g$ . Triangles and asterisks are planet host and comparison sample stars, respectively. Dotted lines represent the solar value. The slopes represent linear least-squares fits to both planet-hosts and comparison stars.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{3850f2.eps} \end{figure}$	Figure 2: Distributions of planet-host stars and non-planet-host stars as functions of $T_{\rm eff}$ . The planet-host stars and the comparison sample are represented with solid and dotted lines, respectively.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3850f3.eps} \end{figure}$	Figure 3: [X/H] distributions for Ti, V and Co for the two subsamples of planet host (solid line) and comparison sample (dotted lines) stars with the same $T_{\rm eff}$ distributions.
Open with DEXTER

$\begin{figure} \par\mbox{\includegraphics[width=5.8cm,clip]{3850f5a.eps}\hspace... ...ps}\hspace{2mm} \includegraphics[width=5.8cm,clip]{3850f5c.eps} }\end{figure}$	Figure 5: [X/H] vs. [Fe/H] for Si, Ca, Ti ( left), for Sc, Mn and V ( centre), for Cr, Co and Ni ( right). Triangles and asterisks represent stars with planetary-mass companion and "single'' field stars, respectively. The intersection of the dotted lines indicates solar value.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=15.6cm,clip]{3850f6.eps} \end{figure}$	Figure 6: [X/H] distribution for each element. The planet-host stars and the comparison sample are represented with solid and dotted lines, respectively.
Open with DEXTER

$\begin{figure} \par\mbox{\includegraphics[width=8.8cm,clip]{3850f7a.eps}\hspace... ...ps}\hspace{2mm} \includegraphics[width=8.8cm,clip]{3850f7d.eps} }\end{figure}$	Figure 7: [X/Fe] vs. [Fe/H](in dex) for $\alpha$ elements (Si, Ca, Ti, Sc) and for iron-peak elements (Cr, Co, Ni, Mn, V). [V/Fe] vs. [Fe/H] for $T_{\rm eff} > 5000$ K objects only ( below right panel). The triangles and asterisks represent stars with planets and "single'' stars, respectively. The intersection of the dotted lines indicates the solar value.
Open with DEXTER

$\begin{figure} \par\mbox{\includegraphics[width=5.6cm,clip]{3850f8a.eps}\hspace... ...ps}\hspace{2mm} \includegraphics[width=5.6cm,clip]{3850f8c.eps} }\end{figure}$	Figure 8: [X/Fe] vs. [Fe/H] trends using binned average values. The bins are 0.2 dex wide, centred on [Fe/H ] =-0.6, -0.4,-0.2,0,0.2 and 0.4 for both samples. Triangles are planet-hosts while rhombi are stars without a planetary-mass companion. The error bars represent the standard deviation about the mean value.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=16cm,clip]{3850f9.eps} \end{figure}$	Figure 9: Same as Fig. 6 but for the Na, Mg and Al distributions.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{3850f11.eps} \end{figure}$	Figure 11: The same as Fig. 8 but for Na, Mg and Al.
Open with DEXTER