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sample-handout.tex
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sample-handout.tex
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\documentclass[handout]{astro-bookshelf}
\hypersetup{colorlinks=true,linkcolor=blue,citecolor=black,urlcolor=blue}
\graphicspath{{Figures/}{frontmatter/}{introduction/figs/}{convection/figs/}{Lane-Emden/figs/}{radiation/figs/}{plasma/figs/}{atmosphere/figs/}{nuclear/figs/}{perturbations/figs/}{binaries/figs/}{technical-notes/figs/}}
\usepackage{aasjournals}
\usepackage{starType}
% symbols used in this work
\newcommand*{\ssb}{\ensuremath{\sigma_{\mathrm{SB}}}} %Stefan-Boltzmann constant
\newcommand*{\rn}{\ensuremath{r_{\mathrm{N}}}} %nuclear radius
\newcommand*{\re}{\ensuremath{r_{\mathrm{E}}}} %classical turning point
\newcommand*{\EG}{\ensuremath{E_{\mathrm{G}}}} %Gamow energy
\newcommand*{\Epk}{\ensuremath{E_{\mathrm{pk}}}} %Peak energy for reaction
\newcommand*{\TPstar}{\left.\frac{\dif T}{\dif P}\right|_{\star}} % derivative of T wrt P in star
\newcommand*{\sun}{\ensuremath{\odot}} %sun
\newcommand*{\eF}{\ensuremath{\varepsilon_{\mathrm{F}}}} %Fermi energy
% vector macros
\newcommand*{\unitvector}[1]{\ensuremath{\bvec{\hat{#1}}}}
\newcommand*{\unitn}{\unitvector{n}} %unit 'n' vector
\newcommand*{\unitk}{\unitvector{k}} %unit 'k' vector
\newcommand*{\unitj}{\unitvector{\jmath}} %unit 'j' vector
\newcommand*{\vu}{\ensuremath{\bvec{u}}} %vector 'u'
\newcommand*{\vv}{\ensuremath{\bvec{v}}} %vector 'v'
\newcommand*{\vx}{\ensuremath{\bvec{x}}} %vector 'x'
\newcommand*{\vr}{\ensuremath{\bvec{r}}} %vector 'r'
\newcommand*{\vg}{\ensuremath{\bvec{g}}} %vector 'g'
\newcommand*{\vp}{\ensuremath{\bvec{p}}} %vector 'p'
\newcommand*{\vk}{\ensuremath{\bvec{k}}} %vector 'k'
\newcommand*{\vkt}{\ensuremath{\bvec{k}_{t}}} %vector 'k_{t}'
\newcommand*{\vxi}{\ensuremath{\bvec{\xi}}} %vector 'k'
\newcommand*{\usp}{\unitskip}
\newcommand*{\nsp}{\usp}
\newcommand*{\maintitle}{Stellar\\Astrophysics}
\newcommand*{\notice}{\thanks{Excerpt from \maintitle, git version \input{git-info}\ldots. Part of the Open Astrophysics Bookshelf; \ccCopy\ 2015 Edward Brown; \ccbyncsa Except where explicitly noted, this work is licensed under the Creative Commons
Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA
4.0) license.}}
\publisher{Open Astrophysics Bookshelf}
\author{Edward Brown}
\date{6 June 2015}
\title{The Sun on a Blackboard\notice}
% \title{The Lagrangian Equations of Stellar Structure\notice}
% \title{Convection\notice}
% \title{Polytropes and the Lane-Emden Equation\notice}
% \title{The Equation of State\notice}
% \title{Radiation Transport\notice}
% \title{Transport in a Plasma\notice}
% \title{Stellar Atmospheres\notice}
% \title{Contraction to the Main Sequence\notice}
% \title{Nuclear Physics\notice}
% \title{Hydrogen Burning and the Main Sequence\notice}
% \title{Post-Main Sequence Evolution: Low-mass Stars\notice}
% \title{Stellar Pulsations\notice}
% \title{The Initial Mass Function\notice}
% \title{Binaries\notice}
% \title{Technical Notes\notice}
\begin{document}
\maketitle
\input{introduction/introduction}
% \input{equations/equations}
% \input{convection/convection}
% \input{Lane-Emden/Lane-Emden}
% \input{eos/eos}
% \input{radiation/radiation}
% \input{plasma/plasma}
% \input{atmosphere/atmosphere}
% \input{PMScontraction/PMScontraction}
% \input{nuclear/nuclear}
% \input{main-sequence/main-sequence}
% \input{post-main-sequence/post-main-sequence}
% \input{perturbations/perturbations}
% \input{initial-mass-function/initial-mass-function}
% \input{binaries/binaries}
% \input{technical-notes/technical-notes}
\bibliographystyle{plainnat}
\bibliography{bibs/stellar}
\end{document}