
<UL>
<LI><A NAME="tex2html27"
 HREF="aa11741-09.right.html">Granulation in K-type dwarf stars</A>
<LI><A NAME="tex2html28"
 HREF="aa11741-09.right.html#SECTION00020000000000000000">1 Introduction</A>
<LI><A NAME="tex2html29"
 HREF="aa11741-09.right.html#SECTION00030000000000000000">2 The 3D model</A>
<LI><A NAME="tex2html30"
 HREF="aa11741-09.right.html#SECTION00040000000000000000">3 Spectrum synthesis in 3D</A>
<LI><A NAME="tex2html31"
 HREF="aa11741-09.right.html#SECTION00050000000000000000">4 Disk-averaged line profiles</A>
<LI><A NAME="tex2html32"
 HREF="aa11741-09.right.html#SECTION00060000000000000000">5 Comparison to observations</A>
<LI><A NAME="tex2html33"
 HREF="aa11741-09.right.html#SECTION00070000000000000000">6 Conclusions</A>
<LI><A NAME="tex2html34"
 HREF="aa11741-09.right.html#SECTION00080000000000000000">Appendix A: The advanced spectrum synthesis 3D tool (Ass<IMG
 WIDTH="10" HEIGHT="26" ALIGN="MIDDLE" BORDER="0"
 SRC="img21.png"
 ALT="$\epsilon $">t)</A>
<LI><A NAME="tex2html35"
 HREF="aa11741-09.right.html#SECTION00090000000000000000">Appendix B: The projected rotational velocity  of HIP&nbsp;86&nbsp;400</A>
<LI><A NAME="tex2html36"
 HREF="aa11741-09.right.html#SECTION000100000000000000000">References</A>
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