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Introducing two improved methods for approximating radiative cooling in hydrodynamical simulations of accretion discs (2024)

First Author: Young A

Attributed to: DiRAC 2.5 Operations 2017-2020 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2405.05762

Publication URI: https://arxiv.org/abs/2405.05762

Type: Preprint