Page 10: Research news on Milky Way Galaxy

The Milky Way Galaxy as a research area encompasses the observational and theoretical study of the structure, dynamics, composition, and evolution of our home galaxy as an astrophysical system. It integrates stellar populations, interstellar medium phases, dark matter halo properties, star formation processes, central supermassive black hole activity, and Galactic chemical evolution. Research focuses on mapping its spiral structure, bar and bulge morphology, disk thickening, satellite interactions, and accretion history using multiwavelength surveys, astrometry, spectroscopy, and numerical simulations. This area provides a detailed laboratory for testing models of galaxy formation and evolution under ΛCDM cosmology, leveraging precise distance scales and resolved stellar populations unique to the Milky Way.

The most distant twin of the Milky Way ever observed

An international team led by the University of Geneva (UNIGE) has discovered the most distant spiral galaxy candidate known to date. This ultra-massive system existed just one billion years after the Big Bang and already ...

Hubble spots star cluster NGC 346

In anticipation of the upcoming 35th anniversary of the NASA/ESA Hubble Space Telescope, ESA/Hubble is kicking off the celebrations with a new image of the star cluster NGC 346, featuring new data and processing techniques. ...

Image: Hubble captures the Small Magellanic Cloud

Say hello to one of the Milky Way's neighbors! This NASA/ESA Hubble Space Telescope image features a scene from one of the closest galaxies to the Milky Way, the Small Magellanic Cloud (SMC). The SMC is a dwarf galaxy located ...

page 10 from 15