$\begin{figure} \par\includegraphics[width=0.283\textwidth]{3794fi1a.eps}\hspace*... ...s}\hspace*{3mm} \includegraphics[width=0.30\textwidth]{3794fi1c.eps}\end{figure}$ Figure 1: Stokes spectra of the Herbig Ae star HD 31648: Normalised Stokes I spectrum ( left) and Stokes V/I spectrum over the full range ( centre) and around the Ca II doublet and nearby H Balmer lines ( right). Zeeman signatures are clearly seen at the locations of the Ca II H and K and H Balmer lines.
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In the text

$\begin{figure} \par\includegraphics[width=0.283\textwidth]{3794fi2a.eps}\hspace*... ...s}\hspace*{3mm} \includegraphics[width=0.30\textwidth]{3794fi2c.eps}\end{figure}$ Figure 2: Stokes spectra of the Herbig Ae star HD 190073: Normalised Stokes I spectrum ( left) and Stokes V/I spectrum over the full range ( centre) and around the Ca II doublet and nearby H Balmer lines ( right). The spectrum is extremely rich in emission lines demonstrating the presence of a strong stellar wind and a dense circumstellar disk. Zeeman signatures are clearly seen in the Ca II H and K lines, but they are not detectable at the locations of the H Balmer lines.
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In the text

$\begin{figure} \par\includegraphics[width=0.42\textwidth]{3794fi3.eps} \end{figure}$ Figure 3: Observed profiles of Ca II H and K in the high resolution spectrum ( $R\sim 48000$ ) of HD 190073 using the FEROS spectrograph (Pogodin et al. 2005).
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In the text

$\begin{figure} \par\includegraphics[width=0.283\textwidth]{3794fi1a.eps}\hspace... ...s}\hspace{3mm} \includegraphics[width=0.30\textwidth]{3794fi1c.eps}\end{figure}$	Figure 1: Stokes spectra of the Herbig Ae star HD 31648: Normalised Stokes I spectrum ( left) and Stokes V/I spectrum over the full range ( centre) and around the Ca II doublet and nearby H Balmer lines ( right). Zeeman signatures are clearly seen at the locations of the Ca II H and K and H Balmer lines.
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$\begin{figure} \par\includegraphics[width=0.42\textwidth]{3794fi3.eps} \end{figure}$	Figure 3: Observed profiles of Ca II H and K in the high resolution spectrum ( $R\sim 48000$ ) of HD 190073 using the FEROS spectrograph (Pogodin et al. 2005).
Open with DEXTER