ARTEMIS simulations
ARTEMIS simulations
Oct 20, 2020
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• Formation of a Massive "Late-type", Star-Forming Disk Galaxy 18.6.2022 VIDEO: Formation of a massive "late-type", star-forming disk galaxy: an individual system is tracked through time, and its stellar light is shown in a 500 kilo-parsec region. This galaxy exhibits rapid ongoing star formation in an extended, clumpy disk, until it experiences a late-time merger (at approximately z ~ 0.3) with a nearly equal mass companion. (01:24) [TNG Simulations] • The IllustrisTNG project is a suite of sta
1:24
• Formation of a Massive "Late-type", Star-Forming Disk Galaxy 18.6.2022 VIDEO: Formation of a massive "late-type", star-forming disk galaxy: an individual system is tracked through time, and its stellar light is shown in a 500 kilo-parsec region. This galaxy exhibits rapid ongoing star formation in an extended, clumpy disk, until it experiences a late-time merger (at approximately z ~ 0.3) with a nearly equal mass companion. (01:24) [TNG Simulations] • The IllustrisTNG project is a suite of sta
2.3K viewsJun 19, 2022
FacebookAstronomy Nation
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
1:50
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
8.5M viewsMay 19, 2019
FacebookAstronomy Nation
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