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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.  \begin{quote}  In the paper, \citet{fuller} show for the first time how internal gravity waves waves,  excited in the turbulent layers of stars at least ten times more massive larger  than the Sun, can radically change their internal rotation rate. In particular particular,  these waves, waves –  somewhat analogous to ocean waves, waves –  can determine how rapidly the stellar core spins around its axis when the star is about to die and become a supernova. The spin of a  pre-supernova cores core  is important because can it  deeply affect affects  the stellar explosion and determine determines  the rotation rate of the stellar remnant (neutron star or black hole). \end{quote}