All Figures

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{1505fig1.ps}\end{figure}$ Figure 1: V and NIR spectra of Luichewoo, Baetsle, and Sofala. For Baetsle and Sofala, the spectra (a) include V data obtained at NTT and NIR spectra obtained at IRTF, while spectra (b) have been obtained at TNG. All the spectra are normalized at 0.55 $\mu$ m and shifted by 0.7 for clarity. All these objects have been classified as S-type.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{1505fig2.ps} \end{figure}$ Figure 2: V spectrum of Lutetia, and V and NIR spectra of Izvekov, Carrera, Rhodia, and Steins. The NIR spectrum (a) of Rhodia has been obtained on January 2004, while the NIR spectrum (b) has been obtained on March 2004. The V spectrum (b) of Steins has been obtained on May 2004. All the spectra are normalized at 0.55 $\mu$ m and shifted by 0.6 for clarity.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,angle=0]{1505fig3.ps}\end{figure}$ Figure 3: Comparison of the Lutetia spectra (our V spectrum + the NIR one by Birlan et al. 2004) and the spectra of the CV3 carbonaceous chondrite meteorite Vigarano.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,angle=0]{1505fig4.ps}\end{figure}$ Figure 4: Comparison of the spectrum of Steins and the spectra of the EL6 enstatite chondrite Atlanta (dashed line), and the enstatite achondrite (aubrite) ALH 78113 (dotted line). All the spectra are normalized at 0.55 $\mu$ m.
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In the text

$\begin{figure} \par\includegraphics[width=8.4cm,clip]{1505fig1.ps}\end{figure}$	Figure 1: V and NIR spectra of Luichewoo, Baetsle, and Sofala. For Baetsle and Sofala, the spectra (a) include V data obtained at NTT and NIR spectra obtained at IRTF, while spectra (b) have been obtained at TNG. All the spectra are normalized at 0.55 $\mu$ m and shifted by 0.7 for clarity. All these objects have been classified as S-type.
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$\begin{figure} \par\includegraphics[width=8.4cm,clip]{1505fig2.ps} \end{figure}$	Figure 2: V spectrum of Lutetia, and V and NIR spectra of Izvekov, Carrera, Rhodia, and Steins. The NIR spectrum (a) of Rhodia has been obtained on January 2004, while the NIR spectrum (b) has been obtained on March 2004. The V spectrum (b) of Steins has been obtained on May 2004. All the spectra are normalized at 0.55 $\mu$ m and shifted by 0.6 for clarity.
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$\begin{figure} \par\includegraphics[width=8.4cm,angle=0]{1505fig3.ps}\end{figure}$	Figure 3: Comparison of the Lutetia spectra (our V spectrum + the NIR one by Birlan et al. 2004) and the spectra of the CV3 carbonaceous chondrite meteorite Vigarano.
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$\begin{figure} \par\includegraphics[width=8.4cm,angle=0]{1505fig4.ps}\end{figure}$	Figure 4: Comparison of the spectrum of Steins and the spectra of the EL6 enstatite chondrite Atlanta (dashed line), and the enstatite achondrite (aubrite) ALH 78113 (dotted line). All the spectra are normalized at 0.55 $\mu$ m.
Open with DEXTER