A team of astrophysicists from Nanjing University and University of Bonn have demonstrated that, rather than being random, ...

The Milky Way may not have a sharp edge, but scientists have now found where its star-forming activity largely comes to an ...

The older stars migrated out from the galactic center, leaving the younger ones inside.

The formation of stars is intricately linked to the complex structure and dynamics of molecular clouds—vast, cold, and dense regions in the interstellar medium that primarily consist of molecular ...

How far the Milky Way's disk extends has long been difficult to define—it doesn't end sharply, but fades away gradually at ...

Created by a young star, the bipolar star-forming region Sharpless 2-106 in this Hubble image depicts how intense the star-formation process can get. When you purchase through links on our site, we ...

Planets, like those in our solar system, form in a bottom-up process where small bits of rock and ice clump together and grow larger over time. But the heftier the planet, the harder it is to explain ...

Starting from the upper left and moving clockwise from large to small scales: upper left —"spiral-like" system; upper right — "bar-like" structure; lower right — rotating infalling envelope; lower ...

For a long time, scientists thought that only actively star-forming galaxies should be observed in the very early Universe. The James Webb space telescope now reveals that galaxies stopped forming ...

How far the Milky Way's disc extends has long been difficult to define — it doesn't end sharply, but fades away gradually at its outer edges. Now, for the first time, an international team of ...