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  How do supernova remnants cool? - I. Morphology, optical emission lines, and shocks

Makarenko, E. I., Walch, S., Clarke, S. D., Seifried, D., Naab, T., Nürnberger, P. C. N., et al. (2023). How do supernova remnants cool? - I. Morphology, optical emission lines, and shocks. Monthly Notices of the Royal Astronomical Society, 523(1), 1421-1440. doi:10.1093/mnras/stad1472.

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Item Permalink: https://hdl.handle.net/21.11116/0000-000D-E5FD-4 Version Permalink: https://hdl.handle.net/21.11116/0000-000D-E5FE-3
Genre: Journal Article

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 Creators:
Makarenko, Ekaterina I., Author
Walch, Stefanie, Author
Clarke, Seamus D., Author
Seifried, Daniel, Author
Naab, Thorsten1, Author           
Nürnberger, Pierre C. N, Author
Rathjen, Tim-Eric, Author
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1Computational Structure Formation, MPI for Astrophysics, Max Planck Society, ou_2205642              

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Language(s): eng - English
 Dates: 2023-05-17
 Publication Status: Published online
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1093/mnras/stad1472
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Title: Monthly Notices of the Royal Astronomical Society
  Other : Mon. Not. R. Astron. Soc.
Source Genre: Journal
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Publ. Info: Oxford : Oxford University Press
Pages: - Volume / Issue: 523 (1) Sequence Number: - Start / End Page: 1421 - 1440 Identifier: ISSN: 1365-8711
CoNE: https://pure.mpg.de/cone/journals/resource/1000000000024150