this is for holding javascript data
Matteo Cantiello edited untitled.tex
over 8 years ago
Commit id: 941afb89433859b073127714e99a8c8dbfe8b940
deletions | additions
diff --git a/untitled.tex b/untitled.tex
index 9820d12..978bfa3 100644
--- a/untitled.tex
+++ b/untitled.tex
...
\section{Steady vs Eruptive Massloss}
To help constrain mass-loss theory, we first need to understand the mass-loss history of massive stars. In particular, we need to know the mass-loss rate ($\dot{M}$) and velocity
($v$) as a function of time before explosion.
The mass loss rates during the last few hundred years of evolution of some core collapse supernova progenitors seem to violate the maximum values allowed by line-driven winds ($\dot{M} \sim 10^{-4}$M$_\odot$yr$^{-1}$, \citet{Smith_2006}, see also Fig.~\ref{fig}).