The chemical enrichment of the Milky Way has a long and complicated history. However that history could be partially explained by the subject of today’s paper: the study of azimuthal variations in its metallicity.
High-velocity stars are interesting both in their origins and in what they can be used to study. Today’s paper takes a brief dive into tackling both of these questions.
What happens when we break a galaxy down to its fundamental building blocks? Today’s authors try to find out!
Dust may not sound very exciting, but it’s incredibly important to astronomy. Today’s authors produce a 3D map of the Milky Way’s dust!
Today’s authors look for the origin of the blobby neutrino emission IceCube sees in the Milky Way!
Today’s authors try to use the behavior of ants to model streams of stars in our galaxy!
