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.

Webb telescope digs into structural origins of disk galaxies

Disk galaxies, like our own Milky Way galaxy, commonly consist of both a thick and thin disk of stars—each with different features, including stellar population and movement. Three major theoretical scenarios have been proposed ...

Hubble spies inclined spiral galaxy NGC 3511

The stately and inclined spiral galaxy NGC 3511 is the subject of this NASA/ESA Hubble Space Telescope image. The galaxy is located 43 million light-years away in the constellation Crater (The Cup). From Hubble's vantage ...