43 lines
1.4 KiB
TeX
43 lines
1.4 KiB
TeX
% !TEX root = ../thesis-example.tex
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%Example chapter on Asteroseismology
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\chapter{Introduction \label{sec:intro}}
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%\cleanchapterquote{Shoot for the moon. Even if you miss, you'll land among the stars.}{Les Brown} %optional, if you want to place something here.
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\section{Current knowledge}
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% motivation for the thesis
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\section{Spectral Types}
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% Different Spectral Types
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\section{Flares and Starspots}
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% Stellar Activity,
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\section{Spacecrafts}
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% TESS, Kepler/K2
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\citet{Thompson2012}.
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\begin{figure}[t!]
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\includegraphics[width=\linewidth]{gfx/rghbHRD.pdf}
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\caption{Position of the 18 red giant heartbeat stars from Tables 1 and 2 in
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the HR diagram, where the colour shows the mass of the red giant, derived from seismology. The size of the dots represents the orbital period,
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ranging between 20 and 438 d. The contour surfaces reflect the density
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distribution of 1000 pulsating red giants. The darkest areas mark the
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position of the densely populated red clump. Numbers in red indicate
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the star count per bin, for which the contour surfaces have been drawn.
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Lines of equal radii in the HR diagram have been drawn for selected
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stellar radii between 5 and 30 R. \citep[Figure taken from][]{Beck2014}}
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\label{fig:singelPanelPlot}
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\end{figure}
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\textit{Kepler} \ref{sec:conclusion}
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\begin{eqnarray}
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c^2 &=& a^2 + b^2, \label{eq:pyth1}\\
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c &=& \sqrt{a^2 + b^2} \label{eq:pyth2},
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\end{eqnarray}
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