Research news on Galaxy disks

Galaxy disks as a research area focuses on the structure, dynamics, formation, and evolution of the flattened, rotationally supported components of galaxies, particularly spiral and lenticular systems. Studies address stellar and gas kinematics, angular momentum distribution, and the interplay between baryons and dark matter in shaping disk profiles (e.g., exponential or broken-exponential). The field investigates disk instabilities, spiral arms, bars, secular evolution, star formation regulation, radial migration, and vertical thickening, often using multiwavelength observations, integral-field spectroscopy, and cosmological simulations. Galaxy disk research is central to constraining galaxy assembly histories, feedback processes, and the coupling between galactic disks, halos, and their broader cosmological environment.

Hubble shows star formation in Andromeda galaxy is winding down

A new study using data from NASA's Hubble Space Telescope finds that star formation in the nearby Andromeda galaxy has undergone a 500-million-year decline, with an even steeper drop in the last 40 million years. Andromeda, ...

Spiral arms and bars are galactic fuel pumps for star formation

Peak star formation took place during cosmic noon, between 2–3 billion years after the Big Bang. The star formation rate (SFR) back then was up to 100 times greater than it is today. For the SFR to be so high, gas had to ...

How a single star can reshape an entire galaxy

Astronomers who simulate galaxies do not always get the same result, even when they start from identical conditions. New research from Leiden University shows that this is not a flaw, but a consequence of how galaxies behave—and ...

page 1 from 3