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Super-Eddington Accretion

The inflow of matter onto a compact object at a rate above the conventional Eddington limit, where outward radiation pressure would normally balance gravity. Thick gas can trap or redirect radiation, allowing faster growth for a time.

English

Super-Eddington Accretion

Arabic

التراكم فوق حد إدنغتون

First appeared in

Webb Finds Strong Evidence for a Black Hole Inside a Solar-System-Sized Gas Cloud

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