We know everything there is to know about the s-process, right? RIGHT?!
A look at how magnetic braking can erase the extended main sequence turn-off feature in old stellar clusters.
We all love lists, especially if they’re short. Here’s one about surviving grad school!
What can we learn from the largest set of neutron star merger simulations with realistic microphysics to date?
What’s behind the phenomenon of extended main sequence turnoffs in star clusters?