Analytical model for non-thermal pressure in galaxy clusters – III. Removing 
the hydrostatic mass bias

Shi, Xun; Komatsu, Eiichiro; Nagai, Daisuke; Lau, Erwin T.

doi:10.1093/mnras/stv2504

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Analytical model for non-thermal pressure in galaxy clusters – III. Removing the hydrostatic mass bias

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Shi, Xun
Physical Cosmology, MPI for Astrophysics, Max Planck Society;

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Komatsu, Eiichiro
Physical Cosmology, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons188873

Nagai, Daisuke
Physical Cosmology, MPI for Astrophysics, Max Planck Society;

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Shi, X., Komatsu, E., Nagai, D., & Lau, E. T. (2016). Analytical model for non-thermal pressure in galaxy clusters – III. Removing the hydrostatic mass bias. Monthly Notices of the Royal Astronomical Society, 455(3), 2936-2944. doi:10.1093/mnras/stv2504.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0029-8157-9

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