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<!-- DOI: 10.1051/0004-6361/200912043 -->

<h2 class="sec">Online Material</h2>
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<h2 class="sec"><a name="SECTION00090000000000000000"></a><A NAME="a:time"></A>
Appendix A: Evolution up to the first TP
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<A NAME="ta:1"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/48/aa12043-09/tableA.1.html"><span class="bold">Table A.1:</span></a>&#160;&#160;
Solar-scaled metallicity models from the ZAMS until the 1
<!-- MATH: $^{{\rm st}}$ --><IMG SRC="img20.png" ALT="$^{{\rm st}}$" align="bottom" BORDER="0" HEIGHT="15" WIDTH="10">
TP. </p>
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<tr><td><!-- init Label --><A NAME="fa:1"></A><!-- end Label--><A NAME="2747"></A><A NAME="figure1949" HREF="img162.png"><IMG SRC="Timg162.png" ALT="\begin{figure}
\par\includegraphics[angle=90,scale=0.3]{12043figA1a.ps}\includeg...
...12043figA1e.ps}\includegraphics[angle=90,scale=0.3]{12043figA1f.ps}
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<td class="img-txt"><span class="bold">Figure A.1:</span><p>
Main sequence lifetimes (<i> left</i>) and core mass at the
first thermal pulse (<i> right</i>) for three chemical
compositions with <i>Z</i>=0.004, 0.008, 0.02 (<i>
from top to bottom</i>) of our models (crosses) in comparison
with literature values from <a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#karakas:2003">Karakas
(2003, K03)</a>,
<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#vasswood:93">Vassiliadis
&amp; Wood (1993, VW93)</a>, and Miller-Bertolami (private
communication, 2008, MB08).
</td>
</tr><tr><td colspan="2"><a href="http://dexter.edpsciences.org/applet.php?pdf_id=17&DOI=10.1051/0004-6361/200912043" target="DEXTER">Open with DEXTER</a></td></tr>

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<p><A NAME="ta:2"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/48/aa12043-09/tableA.2.html"><span class="bold">Table A.2:</span></a>&#160;&#160;
Same as for Table&nbsp;<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#ta:1">A.1</a>
but for the <IMG SRC="img5.png" ALT="$\alpha $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="12">-enhanced
metallicity models.</p>
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<h2 class="sec"><a name="SECTION000100000000000000000"></a><A NAME="a:summary"></A>Appendix B: Summary of AGB properties
</h2>
<A NAME="ta:3"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/48/aa12043-09/tableB.1.html"><span class="bold">Table B.1:</span></a>&#160;&#160;
Same as Table&nbsp;<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#t:4">4</a>,
but for mixtures I and II (Table&nbsp;<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#t:1">1</a>) with <i>Z</i>=0.04.</p>
<p><A NAME="ta:4"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/48/aa12043-09/tableB.2.html"><span class="bold">Table B.2:</span></a>&#160;&#160;
Same as Table&nbsp;<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#t:4">4</a>,
but for mixtures V and VI (Table&nbsp;<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#t:1">1</a>) with <i>Z</i>=0.008.</p>
<p><A NAME="ta:5"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/48/aa12043-09/tableB.3.html"><span class="bold">Table B.3:</span></a>&#160;&#160;
Same as Table&nbsp;<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#t:4">4</a>,
but for mixtures VII and VIII
(Table&nbsp;<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#t:1">1</a>)
with <i>Z</i>=0.004.</p>
<p><A NAME="ta:6"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/48/aa12043-09/tableB.4.html"><span class="bold">Table B.4:</span></a>&#160;&#160;
Same as Table&nbsp;<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#t:4">4</a>,
but for mixtures IX and X (Table&nbsp;<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#t:1">1</a>) with <i>Z</i>=0.0005.</p>
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<h2 class="sec"><a name="SECTION000110000000000000000"></a>Appendix C:
Post-AGB evolution</h2>
<A NAME="ta:7"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/48/aa12043-09/tableC.1.html"><span class="bold">Table C.1:</span></a>&#160;&#160;
Post-AGB evolution for all models with solar-scaled metal distributions
computed through this phase<sup><i>a</i></sup>.
</p>
<p><A NAME="ta:8"></A><p class="inset-old"><a href="/articles/aa/full_html/2009/48/aa12043-09/tableC.2.html"><span class="bold">Table C.2:</span></a>&#160;&#160;
As Table&nbsp;<a href="/articles/aa/full_html/2009/48/aa12043-09/aa12043-09.html#ta:7">C.1</a>,
but for the <IMG SRC="img5.png" ALT="$\alpha $" ALIGN="MIDDLE" BORDER="0" HEIGHT="26" WIDTH="12">-enhanced
composition tracks.</p>
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