deletions | additions       diff --git a/Abstract.tex b/Abstract.tex  index 4a28da8..0a13d2c 100644  --- a/Abstract.tex  +++ b/Abstract.tex 
...
\section{Abstract}  The quality of ALMA observations of stellar outflows are examined using simulations and CASA observations. Various configurations and observations paramters were used to determine how much information about the simulation is returned by each setup. We argue that snapshots are usefull for getting an approximation of the outflow and that more compact arrays give better results for our input. We also show that longer integration pointing  times do not significantly degrade ALMA's results.