Page 13: 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.

Gaia spots odd family of stars desperate to leave home

Stars in the Milky Way tend to form in families, with similar stars springing to life in roughly the same place at roughly the same time. These stars later head out into the wider galaxy when they're ready to fly the nest. ...

What blew up the local bubble?

In our neighborhood of the Milky Way, we see a region surrounding the solar system that is far less dense than average. But that space, that cavity, is a very irregular, elongated shape. What little material is left inside ...

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. ...

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