Simulation of Intergalactic Medium Coalescing and Formation of Proto-cluster. • The IllustrisTNG Project 18.5.2019 VIDEO: (Best Viewed on Large Screen) The motion of cosmic gas in a small region of TNG50, color encoding velocity from at rest (black) to 1000 km/s (bright red and white). At early times, accretion and infall from the intergalactic medium coallesces in the centers of many small halos. Stellar feedback produces slow galactic winds which gradually push mass outwards, until several cen

A Far Away Star Cluster NGC 281 JAN. 27/2018 High-mass stars are important because they are responsible for much of the energy pumped into a galaxy over its lifetime. Unfortunately, these stars aren’t understood very well because they are usually found relatively far away in places where lots of gas and dust impede our view. This star cluster (NGC 281) however, is an exception since it is far enough away from the plane of our galaxy that not a lot of dust and gas obscure its view. The high-mass

Globular star clusters are beautiful to look at, but what exactly are they? Find out in this #StarrySights science lesson! You can learn more about star clusters here, too: https://go.nasa.gov/3uh5cE9 #NASA #Hubble #stars #science #space #astronomy #universe #cosmos #telescope | NASA's Hubble Space Telescope

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