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State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows (2023)

First Author: Higginbottom N

Attributed to: Astrophysics at Southampton funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2312.06042

Publication URI: https://arxiv.org/abs/2312.06042

Type: Preprint