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Image for: Wie schwarze Löcher den Kosmos formen


Visualisierung des Gasgeschwindigkeitsfeldes in einem dünnen Schnitt mit einer Dicke von 100 Kiloparsec. In der Bildmitte ist der zweitschwerste Galaxienhaufen in der TNG100 Simulation zu sehen.
Visualisierung des Gasgeschwindigkeitsfeldes in einem dünnen Schnitt mit einer Dicke von 100 Kiloparsec. In der Bildmitte ist der zweitschwerste Galaxienhaufen in der TNG100 Simulation zu sehen.

IllustrisTNG

(239 KB, 1344 x 756 pixels)

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