How can tides help us find hidden compact companions and yield detailed physics on stellar binaries?
Today’s paper examines if a well-known correlation between gas mass and star formation rate holds on the scale of a single molecular cloud.
Heavy elements require extreme conditions to be produced. Today’s bite explores three unique stars that may give us additional clues on how that happens.
Massive stars live fast and die young, making metals along the way.
Meet Leo I, one of the dwarf galaxies that may help us understand the earliest galaxies to form.