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<!-- DOI: 10.1051/0004-6361/200911657 -->

<h2 class="sec">Online Material</h2>

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<A NAME="table_HD49933_posterior_individual_Frequency_M2A"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/40/aa11657-09/table10.html"><span class="bold">Table 10:</span></a>&#160;&#160;
HD&nbsp;49933 frequencies and height-to-noise posterior estimates for <I>l</I>=0 and <I>l</I>=1&nbsp;modes for the 
<!-- MATH: $M^2_{\rm A}$ -->
<IMG
 WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
 SRC="img11.png"
 ALT="$M^2_{\rm A}$">&nbsp;model. <I>n</I> is given supposing 
<!-- MATH: $\epsilon\in[1,2]$ -->
<IMG
 WIDTH="53" HEIGHT="26" ALIGN="MIDDLE" BORDER="0"
 SRC="img12.png"
 ALT="$\epsilon \in [1,2]$">.
<I>H</I>/<I>N</I> represents the height-to-noise ratio in the power spectrum.</p>
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<A NAME="table_HD49933_posterior_individual_Height_M2A"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/40/aa11657-09/table11.html"><span class="bold">Table 11:</span></a>&#160;&#160;
Height and width posterior estimates for HD&nbsp;49933 for the model 
<!-- MATH: $M^2_{\rm A}$ -->
<IMG
 WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
 SRC="img11.png"
 ALT="$M^2_{\rm A}$">.
<I>n</I> is given for the <I>l</I>=0&nbsp;modes.</p>
<p>
<A NAME="table_HD49933_posterior_individual_Amplitude_M2A"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/40/aa11657-09/table12.html"><span class="bold">Table 12:</span></a>&#160;&#160;
Energy posterior estimates for HD&nbsp;49933, model 
	
<!-- MATH: $M^2_{\rm A}$ -->
<IMG
 WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
 SRC="img11.png"
 ALT="$M^2_{\rm A}$">.
<I>n</I> is given for the <I>l</I>=0&nbsp;modes.</p>
<p>
  
<p>
<A NAME="table_HD49933_posterior_individual_Frequency_M2B"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/40/aa11657-09/table13.html"><span class="bold">Table 13:</span></a>&#160;&#160;
HD&nbsp;49933 frequencies and height-to-noise posterior estimates for the <I>l</I>=0 and <I>l</I>=1&nbsp;modes for the 
<!-- MATH: $M^2_{\rm B}$ -->
<IMG
 WIDTH="22" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
 SRC="img10.png"
 ALT="$M^2_{\rm B}$">&nbsp;model. <I>n</I> is given supposing 
<!-- MATH: $\epsilon\in[1,2]$ -->
<IMG
 WIDTH="53" HEIGHT="26" ALIGN="MIDDLE" BORDER="0"
 SRC="img12.png"
 ALT="$\epsilon \in [1,2]$">.
<I>H</I>/<I>N</I> represents the height-to-noise ratio in the power spectrum.</p>
<p>
<A NAME="table_HD49933_posterior_individual_Height_M2B"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/40/aa11657-09/table14.html"><span class="bold">Table 14:</span></a>&#160;&#160;
Height and width posterior estimates for HD&nbsp;49933 for the model 
<!-- MATH: $M^2_{\rm B}$ -->
<IMG
 WIDTH="22" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
 SRC="img10.png"
 ALT="$M^2_{\rm B}$">.
<I>n</I> is given for the <I>l</I>=0&nbsp;modes.</p>
<p>
<A NAME="table_HD49933_posterior_individual_Amplitude_M2B"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/40/aa11657-09/table15.html"><span class="bold">Table 15:</span></a>&#160;&#160;
Energy posterior estimates for HD&nbsp;49933, model 
<!-- MATH: $M^2_{\rm B}$ -->
<IMG
 WIDTH="22" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
 SRC="img10.png"
 ALT="$M^2_{\rm B}$">.
<I>n</I> is given for the <I>l</I>=0&nbsp;modes.</p>
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<p>

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<tr><td><!-- init Label --><A NAME="fig:spectrum_samples_M2A">&#160;</A><!-- end Label--><A NAME="1681"></A><A NAME="figure1439"
 HREF="img211.png"><IMG
 WIDTH="204" HEIGHT="67" SRC="Timg211.png"
 ALT="\begin{figure}
\par\subfigure{\epsfig{figure=11657_ZD.ps,width=6.cm,height=18cm,angle=90} }
\par
\end{figure}"></A><!-- HTML Figure number: 11 --></td>
<td class="img-txt"><span class="bold">Figure 11:</span><p>
HD&nbsp;49933 power spectrum and echelle diagram for 
<!-- MATH: $M^2_{\rm A}$ -->
<IMG
 WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
 SRC="img11.png"
 ALT="$M^2_{\rm A}$">&nbsp;model (identification A with <I>l</I>=2&nbsp;modes). The superimposed dashed line is the best fit according to the median value of the parameters.</p></td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=11&DOI=10.1051/0004-6361/200911657" target="DEXTER">Open with DEXTER</a></td></tr>

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<tr><td><!-- init Label --><A NAME="fig:spectrum_samples_M1B">&#160;</A><!-- end Label--><A NAME="1683"></A><A NAME="figure1445"
 HREF="img212.png"><IMG
 WIDTH="204" HEIGHT="67" SRC="Timg212.png"
 ALT="\begin{figure}
\par\subfigure{\epsfig{figure=11657_ZE.ps,width=6.cm,height=18cm,angle=90} }
\par
\end{figure}"></A><!-- HTML Figure number: 12 --></td>
<td class="img-txt"><span class="bold">Figure 12:</span><p>
HD&nbsp;49933 power spectrum and echelle diagram for 
<!-- MATH: $M^1_{\rm B}$ -->
<IMG
 WIDTH="23" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
 SRC="img13.png"
 ALT="$M^1_{\rm B}$">&nbsp;model (identification B without <I>l</I>=2&nbsp;modes). The superimposed dashed line is the best fit according to the median value of the parameters.</p></td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=12&DOI=10.1051/0004-6361/200911657" target="DEXTER">Open with DEXTER</a></td></tr>

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