this is for holding javascript data
Jeff Montgomery renamed untitled.tex to intro.tex
about 9 years ago
Commit id: 717a36fd343eb9e2971438277a5efa1afe3fb635
deletions | additions
diff --git a/intro.tex b/intro.tex
new file mode 100644
index 0000000..3a7350b
--- /dev/null
+++ b/intro.tex
...
A recent \href{https://www.authorea.com/users/2/articles/19261/_show_article}{document} was written on Authorea and submitted to the Astrophysical Journal (pre-print pdf now on \href{http://arxiv.org/abs/1502.07779}{arXiv}).
In the meantime, the authors want to test Authorea as a platform for \textbf{open peer-review}. By going to the document's page, you can \href{https://www.authorea.com/users/9932/articles/13560/_show_article}{Comment} on a section, observation, sentence, or the whole piece. The authors and other commenters can respond and further the discussion. And it's all out in the open, \href{https://www.authorea.com/users/3/articles/6316/_show_article}{just how science was meant to be}.
But it doesn't stop there. You can also view full-size, high-resolution versions of the paper's figures, as well as easily follow links in the References at the bottom of the page.
In this paper, Fuller et al present evidence that the internal gravity waves of a large, late stage star can be greatly influenced by the outer conditions of the star itself. The stronger burning and material flux on the surface of the star could potentially cause an increase in the rotational frequency of the star's iron core, prior to the formation of a core collapse supernova. Instead, the authors determine that the core's rotation is slowed due to the periodic nature of the outer shell's burning.
