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

Young, A.K. orcid.org/0000-0001-7414-1648, Celeste, M., Booth, R.A. orcid.org/0000-0002-0364-937X et al. (4 more authors) (2024) Introducing two improved methods for approximating radiative cooling in hydrodynamical simulations of accretion discs. Monthly Notices of the Royal Astronomical Society, 531 (1). pp. 1746-1755. ISSN 0035-8711

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Item Type: Article
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© 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.

Keywords: hydrodynamics, radiative transfer, methods:numerical
Dates:
  • Published: June 2024
  • Published (online): 13 May 2024
  • Accepted: 9 May 2024
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Physics and Astronomy (Leeds) > Astrophysics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 21 May 2024 14:37
Last Modified: 07 Aug 2024 14:32
Status: Published
Publisher: Oxford University Press
Identification Number: 10.1093/mnras/stae1249
Open Archives Initiative ID (OAI ID):

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