Two Paths Diverged in a Cosmological Simulation: on the Formation Pathways of S0 Galaxies
Today’s bite explores the two main pathways of S0 galaxy formation, ram-pressure stripping and galaxy mergers.
Today’s bite explores the two main pathways of S0 galaxy formation, ram-pressure stripping and galaxy mergers.
In the heart of the barred spiral galaxy NGC 1097, there’s more to the magnetic field than meets the eye.
Most galaxies are either star-forming disks, or red, dead spheroids. But, have galaxy clusters now shown that this divide isn’t quite so clear?
The Milky Way’s disc is made up of two components — but where did they come from?
Ever wondered how astronomers study the structure of our own Galaxy from within? Read on to find out how the Gaia mission helps us in this regard!
Major galaxy mergers are thought to be one of the main ways of producing massive elliptical galaxies. Surprisingly though, some of the most massive galaxies in the local universe have gas disks. Here’s how they might be made.