mirror of
https://asciireactor.com/otho/phy-4660.git
synced 2024-11-22 05:25:07 +00:00
images
This commit is contained in:
parent
bb0998fce4
commit
f873d5e5d3
Before Width: | Height: | Size: 21 KiB After Width: | Height: | Size: 21 KiB |
@ -56,7 +56,7 @@
|
||||
|
||||
\begin{figure}
|
||||
\center
|
||||
\includegraphics[width=4.5in]{../abundances.png}
|
||||
\includegraphics[width=4.5in]{abundances.png}
|
||||
\caption{Relative elemental abundances in the sun's photosphere. Lithium and fluorine are much less abundant than their neighbour elements. It is thought this is due to large probability cross-sections for a proton collision with these nuclei. \cite{Carroll&Ostlie}}
|
||||
\label{fig:abundances}
|
||||
\end{figure}
|
||||
@ -72,7 +72,7 @@
|
||||
|
||||
\begin{figure}
|
||||
\center
|
||||
\includegraphics{}
|
||||
\includegraphics[width=4.5in]{detector.jpg}
|
||||
\end{figure}
|
||||
|
||||
|
||||
|
Loading…
Reference in New Issue
Block a user