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\BOOKMARK [1][-]{section.1}{Einleitung}{}% 1
\BOOKMARK [2][-]{subsection.1.1}{Themen}{section.1}% 2
\BOOKMARK [2][-]{subsection.1.2}{Motivation}{section.1}% 3
\BOOKMARK [1][-]{section.2}{Hauptteil}{}% 4
\BOOKMARK [2][-]{subsection.2.1}{Notes}{section.2}% 5
\BOOKMARK [3][-]{subsubsection.2.1.1}{Todo}{subsection.2.1}% 6
\BOOKMARK [3][-]{subsubsection.2.1.2}{Generally building a galaxy}{subsection.2.1}% 7
\BOOKMARK [3][-]{subsubsection.2.1.3}{Spiral Galaxy}{subsection.2.1}% 8
\BOOKMARK [3][-]{subsubsection.2.1.4}{Important aspects of spiral galaxies}{subsection.2.1}% 9
\BOOKMARK [3][-]{subsubsection.2.1.5}{Speed}{subsection.2.1}% 10
\BOOKMARK [2][-]{subsection.2.2}{Navarro\205Frenk\205White profile}{section.2}% 11
\BOOKMARK [2][-]{subsection.2.3}{Einasto profile}{section.2}% 12
\BOOKMARK [2][-]{subsection.2.4}{Blender + Python}{section.2}% 13
\BOOKMARK [2][-]{subsection.2.5}{Making things faster}{section.2}% 14
\BOOKMARK [2][-]{subsection.2.6}{Spiral Galaxies}{section.2}% 15
\BOOKMARK [3][-]{subsubsection.2.6.1}{N-K\366rper problem}{subsection.2.6}% 16
\BOOKMARK [3][-]{subsubsection.2.6.2}{Hilbert Spiral}{subsection.2.6}% 17
\BOOKMARK [2][-]{subsection.2.7}{Gr\366\337eneinheiten}{section.2}% 18
\BOOKMARK [1][-]{section.3}{Ergebnisse}{}% 19
\BOOKMARK [2][-]{subsection.3.1}{Simulation Speed}{section.3}% 20
\BOOKMARK [2][-]{subsection.3.2}{Spiral Galaxies}{section.3}% 21
\BOOKMARK [2][-]{subsection.3.3}{Distortion of Galaxies}{section.3}% 22
\BOOKMARK [1][-]{section.4}{Quellen und Hilfen}{}% 23
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