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.

doi:10.1093/mnras/sty2390

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

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Sanders, J. S.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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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.

Cite as: https://hdl.handle.net/21.11116/0000-0003-2740-9

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