Galaxy mergers represent a transformative evolutionary path, inducing notable morphological and compositional changes in the involved galaxies. The alterations in the intrinsic characteristics during these collisions serve as a crucial probe, providing insights into the real-time occurrence of such processes.
Over time, the universe evolved from a primordial soup of hydrogen and helium into the metal-rich environments of today. How exactly does the chemistry of galaxies evolve, and what processes drive this evolution?
This bite reports a serendipitous discovery of what is possibly the largest protoplanetary disk, which has an interesting shape.
What do neutrinos and soccer games have in common? Check out today’s bite to see! Spoiler: starbursts lose the neutrino production game!
Astronomers will literally see a very young star running away from its peers and call it a RATT.
What can local metal-poor stars teach us about the earliest stars in the universe?