Giving Stars a Brake
Stars of various temperatures and sizes slow down at different rates– and to different extents. The authors of this paper address this distinction in a regime never before addressed observationally.
Asymmetries are red, violets are blue, superflares are seen in white light, and H-alpha too!
We don’t fully understand the emission processes in stellar flares. These authors try to get to the heart of the problem with multi-instrument observations.