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  What fraction of the density fluctuations in the Perseus cluster core is due to gas sloshing rather than AGN feedback?

Walker, S. A., Sanders, J. S., & Fabian, A. C. (2018). What fraction of the density fluctuations in the Perseus cluster core is due to gas sloshing rather than AGN feedback? Monthly Notices of the Royal Astronomical Society, 481(2), 1718-1725. doi:10.1093/mnras/sty2390.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0003-2740-9 Version Permalink: https://hdl.handle.net/21.11116/0000-0003-2741-8
Genre: Journal Article

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What fraction of the density fluctuations in the Perseus cluster core is dueto gas sloshing rather than AGN feedback.pdf (Any fulltext), 8MB
 
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Walker, S. A., Author
Sanders, J. S.1, Author           
Fabian, A. C., Author
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1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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 Dates: 2018-09-032018-12
 Publication Status: Issued
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 Rev. Type: Peer
 Identifiers: DOI: 10.1093/mnras/sty2390
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Title: Monthly Notices of the Royal Astronomical Society
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Source Genre: Journal
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Publ. Info: OXFORD : OXFORD UNIV PRESS
Pages: - Volume / Issue: 481 (2) Sequence Number: - Start / End Page: 1718 - 1725 Identifier: ISSN: 0035-8711
CoNE: https://pure.mpg.de/cone/journals/resource/1000000000021470